The galaxy appears as a diffuse, elliptical-like object with a notable central bulge. The light distribution suggests a concentration of older stars, giving it a yellow-reddish hue. There is a secondary concentration of light to one side that seems to be interacting with the main body. A tidal tail or distorted arm cannot be ruled out. The overall morphology points towards a system with reduced star formation activity. The galaxy exhibits a relatively smooth appearance, with no prominent spiral arms visible. It seems to be in the process of merging.
