The galaxy appears to be an elliptical-type galaxy with a largely smooth morphology, though some disturbances are visible. It is generally round in shape but with some irregularities. The galaxy has a reddish hue, suggesting an older stellar population. There is evidence of ongoing merging activity, including a significant disturbance in the main body, which has a somewhat disturbed form, possibly due to tidal interactions. The color is quite red, with the bluest portion being within the inner part of the galaxy. Based on the observed color and morphology, it is likely a massive galaxy that has a moderate amount of star formation, but is primarily composed of older stars.
