The galaxy presents a predominantly smooth morphology, with a notable, somewhat irregular central bulge that appears slightly elongated. The overall shape of the galaxy is moderately round, though not perfectly spherical, displaying a slight departure from circular symmetry. There is evidence of possible interaction or tidal disturbances in the outer regions, and possibly a merger in progress based on the asymmetry and disturbed structure. The presence of a disk cannot be ruled out. The color profile is largely dominated by yellowish hues in the core region, indicative of an older stellar population. Fainter bluish colors in the outer disk suggest the presence of some younger, hotter stars, albeit at a lower overall star formation rate. The dust content appears to be low. Overall, this galaxy appears to be in transition, possibly between a spiral and elliptical morphology.
