The galaxy presents as a relatively smooth object with a concentrated central bulge. It displays a somewhat elliptical morphology, appearing more rounded than elongated. There is a hint of a faint, diffuse disk surrounding the central region, but the disk structure is not prominent. Color gradients suggest a population of older stars dominating the bulge, which appears more reddish or yellowish. The outer regions of the galaxy show bluer hues, possibly indicative of younger stellar populations or ongoing star formation, albeit at a low rate. There is no obvious evidence of major disturbances or tidal features that would suggest a recent major merger event. However, subtle asymmetries or irregularities might indicate minor interactions or internal processes.
