The galaxy presents as a relatively compact object with a noticeable central bulge exhibiting a yellowish hue, suggestive of an older stellar population. Surrounding the core is a less defined, bluer halo. The light distribution is fairly smooth. There is some indication of a possible disk structure in the surrounding halo, though not sharply defined. Faint irregular features are visible in the outer regions suggesting possible recent interactions or internal activity. The galaxy appears moderately massive with ongoing star formation.
