The galaxy appears to be an elliptical galaxy with a smooth, diffuse light distribution. It exhibits a centrally concentrated brightness profile, suggesting a well-defined nucleus. There is little evidence of spiral arm structure or significant dust lanes. The galaxy presents a near-circular morphology, exhibiting a high degree of rotational symmetry. There is no clear indication of any major merging events or tidal disturbances affecting its overall structure, although a possible minor disturbance could be present. The galaxy is yellowish to reddish in color, indicative of an older stellar population with low ongoing star formation.
