The galaxy presents a generally smooth, elliptical morphology, suggesting a classification towards early-type galaxies. Its light distribution appears relatively concentrated, with a high degree of roundness and a lack of prominent spiral arms or bar structures. There is a subtle color gradient observed, with the core appearing somewhat yellower/redder compared to the outer regions, potentially indicating an older stellar population at the galaxy's center. There is no evidence of strong tidal features, major disturbances, or ongoing major mergers. Faint, subtle irregularities may exist within the extended halo, but it is generally indicative of a relaxed system with little recent interaction.
