The galaxy presents as a centrally concentrated object, likely an elliptical or lenticular type. It exhibits a smooth, diffuse light distribution with a high degree of central concentration. The galaxy's shape appears to be moderately elongated, but not extremely so. There is no obvious spiral structure or prominent disk component visible. There is no evidence of ongoing major mergers or significant tidal disturbances, though the galaxy is not perfectly smooth and may have undergone minor interactions in the past. The galaxy presents a consistent color profile, meaning it's likely dominated by an older stellar population.
