The galaxy presents as a somewhat diffuse, elliptical structure, exhibiting a dominant central bulge with a smooth light distribution. There is a noticeable yellow hue, indicative of an older stellar population with fewer blue, high-mass stars. Faint extensions are seen, indicating ongoing or past interactions. There is evidence of asymmetry within the outer halo, suggestive of possible minor disturbances due to tidal interactions. Overall, the galaxy appears to be relatively quiescent, with signs of potential merging activity.
