The galaxy appears to be relatively compact, approximately circular, with a radial extent of ~6 arcseconds. The central region exhibits a bright, concentrated luminosity profile. The overall color profile transitions from blue in the inner region to red towards the outer edges, suggestive of differential stellar populations with younger, bluer stars concentrated towards the core and older, redder stars dominating the outer halo. There are no prominent spiral arms or other distinct morphological features, but slight distortions may be present in the outer regions suggesting minor tidal interactions or disturbances.
