The galaxy presents a disk-like morphology with a prominent central bulge. The bulge appears largely spheroidal and exhibits a yellowish-white color, suggestive of an older stellar population. The disk component is less distinct, potentially exhibiting some spiral arm structure, though this is not entirely clear from the image. The overall color profile suggests a mixed population of stars with a moderate amount of ongoing or recent star formation. There are indications of some disruption in the morphology, possibly due to a minor merger or tidal interaction in the past. Overall, the galaxy appears to be relatively massive and moderately luminous.
