The galaxy presents as a relatively smooth, elliptical-like structure, showing a centrally concentrated light profile with decreasing luminosity outwards. It appears moderately round, lacking a prominent disk or spiral arm features. The color indices suggest an evolved stellar population, indicative of older, redder stars, with a possible lower rate of on-going star formation. There is a slight suggestion of a minor disturbance or interaction occurring, although the primary galaxy body remains largely undisturbed.
