The galaxy appears to be a relatively compact object, exhibiting a primarily smooth morphology with some features that suggest a possible disk-like structure. Its overall shape is neither perfectly round nor distinctly cigar-shaped, but rather somewhere in between, showing a mild elongation. The light distribution suggests a central bulge. There is evidence of subtle disturbances in the galaxy's structure, possibly indicative of minor interactions or internal dynamic processes, with a non-negligible probability of a recent or ongoing merger event. Color gradients within the galaxy hint at variations in stellar populations or dust content, with a bluer hue apparent towards the outer regions and a more yellow-orange tone in the central region.
