The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge which seems to gradually fade outwards. The core of the galaxy displays a yellow-orange hue, indicative of an older stellar population. The outer regions of the galaxy appear slightly bluer, possibly suggesting the presence of some younger, hotter stars, but the light is dominated by a redder population. There is no obvious spiral arm structure or distinct dust lanes visible in the image. The overall shape is highly circular, and there does not appear to be any indication of active merging or significant tidal disturbances affecting the galaxy. The galaxy has a moderate redshift, placing it at a considerable distance.
