The galaxy presents a generally smooth, elliptical morphology. It is not perfectly spherical, exhibiting a slight elongation. The light distribution is concentrated towards the center, suggesting a prominent bulge. There is some subtle internal structure, potentially faint spiral arms or dust lanes. The galaxy appears moderately massive. The color profile suggests a population of older stars, with a reddish-yellow hue dominating. Star formation activity appears low. There's no visual evidence of a recent or ongoing major merger, though subtle disturbances indicate possible minor interactions. Overall, the galaxy looks to be in a relatively evolved state.
