The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated, bright core, transitioning outwards to a more diffuse halo. Color gradients suggest a population of older stars dominating the core, displaying a redder hue, while bluer tones are observed in the outer regions, possibly indicating ongoing, though relatively low, star formation activity within a disk. There is no clear indication of strong spiral arm structure or major disturbances due to recent mergers. Subtle irregularities in the outer halo may suggest minor past interactions or tidal effects. The object appears moderately massive with a relatively low specific star formation rate.
