The galaxy exhibits a centrally concentrated light distribution, with a relatively compact core region that appears bright and somewhat unresolved. The overall morphology is broadly elliptical, though there are some asymmetries visible in the extended halo. The central region has a blue-green hue, indicating active star formation. The outer regions, especially to the lower left, display a fainter, reddish-yellow coloration, suggesting an older stellar population. There appears to be some minor tidal disturbance or interaction, based on some fuzzy asymmetry in the outer halo, but not a major merger.
