The galaxy presents a generally smooth morphology, with a somewhat elliptical shape. It exhibits a concentrated central bulge that dominates its overall light profile. A faint, diffuse halo surrounds the central region, gradually fading into the background. Color gradients are noticeable; the core appears yellowish, potentially indicating an older stellar population, while the outer regions show a slightly bluer hue, suggestive of more recent star formation activity, albeit at a relatively low rate. There is no apparent spiral structure or distinct dust lanes visible. The galaxy appears relatively undisturbed, with no major signs of tidal interactions or ongoing mergers.
