This galaxy presents an elongated, cigar-shaped morphology, suggestive of an elliptical classification. The light distribution appears relatively smooth and centrally concentrated, with a redder hue dominating the central region, potentially indicating an older stellar population. A faint disk is observed, exhibiting slightly bluer colors that may indicate the presence of ongoing or recent star formation. There is no visual evidence of major mergers or significant disturbances in the galaxy's structure.
