The galaxy presents a primarily smooth morphology. Its shape appears to be oblate, leaning towards an elliptical form. The galaxy exhibits a concentration of light toward the center, suggesting a prominent galactic bulge. The color profile indicates a dominant yellowish hue in the central region, possibly indicative of an older stellar population. A faint blue tint is observable in the outer regions, potentially signaling areas of more recent star formation activity, though limited. There is no obvious distortion or tidal features visible, indicating it is likely not undergoing a major merging event. There is a very slight asymmetry in the overall shape which suggests a possible minor disturbance.
