The galaxy presents a generally smooth, elliptical morphology with a prominent central bulge. The color gradient suggests a population of older stars dominating the bulge region, appearing more yellow-orange. A faint, diffuse disk surrounds the bulge, exhibiting a bluer hue, which could indicate the presence of younger stars and ongoing star formation, albeit at a modest rate. There is no distinct spiral arm structure or bar visible. The overall shape leans toward an oblate spheroid, with a possible slight deviation suggesting a mild interaction or tidal disturbance, but no clear signs of a major merger event are apparent. The size appears moderately large, suggesting a massive galaxy.
