The galaxy presents as an elliptical morphology, appearing largely smooth and rounded. The central region exhibits a concentrated luminosity, indicative of a substantial stellar population. The color gradient suggests an older stellar population, with a redder hue towards the center. There is minimal indication of spiral arm structures or significant dust lanes. Weak tidal features are visible. It is likely undergoing minor gravitational interaction. Overall, the galaxy presents a morphology consistent with an early-type galaxy experiencing minor disturbances.
