The galaxy presents as an elliptical morphology, exhibiting a smooth, centrally concentrated luminosity profile. The galaxy's overall color is yellowish, indicative of an older stellar population. The axial ratio suggests a moderate ellipticity. There is no evidence of significant spiral arm structure or prominent dust lanes. Subtle bluer regions are present at its outermost parts, these could potentially indicate regions of ongoing star formation. There does not appear to be any major interactions or merging activity impacting its overall structure.
