The galaxy presents as a moderately luminous object with an elliptical morphology. The light distribution appears relatively smooth, with a concentrated central region and a gradual decline in brightness towards the outer edges. There are no prominent spiral arms or a distinct disk structure visible, suggesting a possible early-type classification. The galaxy's color index indicates a population dominated by older stars, with some contribution from younger stars that are still forming. The overall structure appears undisturbed, with no signs of major mergers or tidal disruptions. However, closer inspection reveals minor irregularities in the outer regions, which may suggest recent interactions or accretion events. Overall, this galaxy seems to be a somewhat massive, relatively evolved system, with ongoing though modest star formation activity.
