The galaxy presents as a relatively smooth, elliptical-like structure with a high degree of central concentration. It appears largely featureless in this observation. The color profile is slightly redder, suggesting a population of older stars. There is no obvious dust lane or spiral arm structure visible. No active galactic nucleus is visually apparent. The galaxy exhibits a generally rounded morphology. There is no strong evidence of ongoing major merging activity. The galaxy may potentially display minor disturbance features, which could indicate recent or ongoing minor interactions.
