The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution appears centrally condensed with a noticeable decrease in intensity towards the outer regions. Hints of a subtle disk-like component may exist, but these features are not prominent. The galaxy appears relatively isolated, with no immediate indications of major mergers or significant tidal disturbances, although minor interactions cannot be ruled out. Color gradients are present, suggesting variations in stellar populations, with the central bulge displaying a more reddish hue compared to the somewhat bluer, fainter outskirts. This color difference could be due to older stellar populations and dust accumulation in the central regions. The overall form indicates a galaxy with a moderate stellar mass and star formation rate.
