The galaxy presents as an elongated, cigar-shaped object with a smooth, diffuse appearance. A central bulge exhibits a brighter, concentrated luminosity, gradually fading into the outer regions of the galaxy. The color gradient suggests a relatively older stellar population. The lack of distinct spiral arms or irregular features points towards a disk-dominated morphology with low active star formation. There is no evidence of any ongoing mergers or major disturbances. The overall morphology suggests an early-type spiral or lenticular galaxy viewed at a significant inclination, but no dust lanes are apparent in this image.
