The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge. The color profile appears to be relatively uniform across the galaxy, with a subtle reddening towards the core, suggesting a population of older stars. There is no apparent spiral structure or significant dust lanes visible in this image. The galaxy appears fairly isolated, showing no obvious signs of tidal interactions or major disturbances that would indicate an ongoing or recent merger event, although very minor asymmetries might be present. The overall rounded shape dominates, with only a slight hint of elongation. The galaxy exhibits a relatively compact size.
