The galaxy presents as a relatively smooth, elliptical object with a concentrated central bulge. It is slightly elongated but generally rounded in shape. The galaxy exhibits a yellowish-red hue, suggesting a population of older stars and a lower rate of ongoing star formation. There are no apparent spiral arm structures or prominent dust lanes visible. The overall morphology indicates a system that is not undergoing any significant merging events or major disturbances. The light appears to be smoothly distributed throughout the galaxy, with a gradual fading towards the edges, suggesting an evolved system with a dominant spheroidal component.
