The galaxy appears to be a relatively smooth, isolated object. It has an elliptical morphology, displaying an elongated shape without prominent spiral arms or a distinct disk structure. There is a subtle color gradient observed, with a slightly bluer hue on the outer edges transitioning to a yellower, more concentrated core. The light distribution suggests a centrally concentrated luminosity profile. No major disturbances or signs of ongoing mergers are readily apparent, although there is a second smaller object nearby that could be interacting with it. 
