The galaxy presents an elliptical morphology, with an apparent disruption in its structure. The central region appears bright and concentrated, indicative of a significant stellar population. Moving outward, the light gradually diminishes into what appears to be a relatively smooth halo. There are indications of a tidal tail on one side of the galaxy, suggesting a past or ongoing interaction with another galaxy. The overall color is yellowish-white, implying a population of older stars, though bluer tinges are visible in some areas. Overall, the galaxy shows a complex morphology, possibly indicating an advanced stage in a merger process.