The galaxy presents as a relatively smooth elliptical, exhibiting a moderate degree of flattening. The central bulge appears bright and concentrated, indicative of a high stellar density. The isophotes are elliptical in shape, with a slight twist evident in the outer regions. The galaxy displays a yellowish-white hue, suggesting a population of older stars with lower star formation activity. No prominent dust lanes or spiral arm structures are discernible in this image. The galaxy appears to be relatively isolated, with no obvious signs of tidal interaction or merging activity. The outer halo appears faint and diffuse, gradually fading into the background. Overall, the morphology suggests a mature, quiescent galaxy likely composed primarily of older stellar populations.
