The galaxy presents as a generally smooth, elliptical structure, with a noticeable lack of distinct spiral arms or prominent features indicative of active star formation regions. The galaxy exhibits a centrally concentrated luminosity, with the light intensity decreasing gradually outwards from the core. The color gradient suggests a relatively old stellar population, with a dominance of redder wavelengths. The galaxy displays a moderate ellipticity, leaning toward a cigar shape. No signs of ongoing major mergers or significant tidal disturbances are apparent. The estimated size suggests that this galaxy is a sizeable structure. The smooth appearance indicates that this galaxy is likely a relatively quiescent system, having largely exhausted its gas reservoir for active star formation.
