The object appears to be a relatively compact galaxy with a high degree of central concentration. It exhibits a generally smooth morphology with a bright, prominent core. The shape is largely elliptical, approaching circular. There may be some minor visual distortions, but generally lacks any significant signs of tidal interactions.

Based on the color profile, there may be a population of older stars dominating the stellar content, particularly in the central region. The outer regions suggest that there could be some ongoing or recent star formation, giving it a slightly bluer hue. There appears to be a potential for a small companion galaxy to be nearby, which is smaller and fainter.
