The galaxy presents as a largely smooth, elliptical morphology. It exhibits a concentrated, bright central bulge, which is a yellow-ish white hue, suggesting an older stellar population. The galaxy displays a gradual decrease in luminosity from its center towards its outer edges. There is little evidence of prominent spiral arms or significant dust lanes. The overall shape appears relatively round, with minimal distortions or tidal features suggestive of recent major merger events. There may be some low-level star formation activity occurring, although at a very subdued rate.
