The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge, with a gradual decrease in luminosity moving outwards. The overall shape is nearly circular. There is a suggestion of minor asymmetry in the outer regions of the galaxy, however, there is no clear evidence of tidal features or ongoing major mergers. The galaxy exhibits a color gradient, with the core appearing more yellow/red, suggestive of an older stellar population. The outer regions are slightly bluer, which may indicate more recent, although minimal, star formation. The galaxy does not show any prominent spiral arm structures or a well-defined disk component. The size is compact, spanning approximately 5 kpc.
