The galaxy presents as an elliptical-like structure, exhibiting a smooth, centrally concentrated luminosity profile with a high degree of roundness. There is little evidence of significant disk features or spiral arms. A dominant central bulge appears to be present, with the light intensity decreasing gradually towards the outer edges. There are no indications of major mergers or significant tidal disturbances, although the possibility of minor interactions cannot be entirely ruled out given the image resolution. The galaxy appears to be generally quiescent, without strong indications of recent or ongoing star formation as inferred from the color profile. The galaxy's light is redder in the central regions and slightly bluer towards the outer edges.
