The galaxy presents an elliptical morphology, appearing somewhat cigar-shaped in projection. There is a high degree of central concentration of light, with a smooth, diffuse halo extending outwards. The color profile suggests a dominant population of older stars, with a subtle gradient toward redder hues in the core. Faint hints of bluer regions are possibly present, suggesting ongoing, but limited, star formation. No obvious spiral arm structure is evident, and there is no indication of a major merger event in its recent history, although minor disturbances cannot be ruled out given the slight asymmetry in its outer regions.
