The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The light distribution appears centrally peaked, fading gradually towards the outer regions of the galaxy. There is a slight elongation, giving it a somewhat cigar-shaped appearance, but it is predominantly round. The colour profile suggests an older stellar population, with a yellow-red hue dominating the core region, potentially indicative of a lack of significant recent star formation. There are no discernible spiral arms or prominent dust lanes visible. There are no indications of strong tidal interactions or major disturbances in the galaxy's morphology.
