The galaxy presents as a luminous, elongated structure, consistent with a disk galaxy viewed at a significant inclination. The central region exhibits a bright, concentrated bulge that appears to be composed of older stellar populations, indicated by its yellowish-white hue.  A faint, extended disk surrounds the bulge, showing some evidence of spiral arm structure, albeit somewhat diffused and indistinct. The disk appears relatively smooth. There is some indication of dust lanes or obscuring material along the periphery of the disk, particularly on the lower left side, but these features are subtle.  The overall morphology suggests a galaxy that is neither purely elliptical nor a grand design spiral, but rather a galaxy with intermediate characteristics, possibly an early-type spiral or a lenticular galaxy. The presence of a well-defined bulge and a visible, though subtle, disk points away from being purely elliptical. There are faint, blueish irregular structures present on the lower left of the disk, implying some form of mild disruption or possible star forming regions. Based on the color index, moderate star formation is present, but not at an extreme rate.
