The galaxy presents as a relatively compact object, approximately 8 kpc in effective radius. Its morphology appears largely spheroidal, with a high degree of smoothness, although there is some indication of subtle structure. The central region exhibits a concentrated luminosity, appearing yellow-white indicating an older stellar population. The outer regions of the galaxy show a bluer tint, possibly indicating regions of more recent star formation. There is a slight asymmetry, with a faint extension emanating from one side, suggesting a potential tidal interaction or minor disturbance, although it does not appear to be undergoing a major merger. The overall impression is that of a massive galaxy with a complex star formation history and some evidence of interaction.
