The galaxy presents as a yellowish-white elliptical, with a smooth, diffuse light distribution, indicative of an older stellar population and minimal dust obscuration. The central region appears slightly more concentrated. There are some minor disturbances that hint at the possibility of a past or ongoing minor merger or tidal interaction. The galaxy exhibits a relatively round morphology, showing only a slight deviation from a circular shape. Overall, the galaxy appears to be relatively isolated, exhibiting no signs of major interaction with neighboring galaxies.
