The galaxy presents as a centrally concentrated object with a generally smooth appearance. The core exhibits a bright, unresolved nucleus, surrounded by a more diffuse halo of light. The overall morphology appears elliptical or spheroidal, lacking prominent spiral arm structures. Color gradients suggest a population of older stars, possibly with ongoing low-level star formation evidenced by a hint of bluer regions within the broader halo. There's a subtle asymmetry in the outer regions, hinting at a possible minor gravitational interaction or past merger event, though no strong tidal features are immediately apparent. The galaxy shows a relatively compact structure, appearing moderately massive and consistent with a passive evolution scenario.
