The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central region, suggesting a substantial bulge component. The overall color appears somewhat blue, possibly indicative of ongoing or recent star formation, although the smoothness suggests this is likely minimal and centrally located. There is little to no apparent spiral arm structure or dust lane obscuration. The light distribution fades gradually towards the outer edges. The galaxy appears undisturbed, with no major signs of interaction or merging events. The overall shape is somewhat rounded, not highly elongated or cigar-shaped. Minor distortions are present, implying a weak interaction with another object, or the remnants of a previous, ancient merger.
