The galaxy exhibits a generally elliptical morphology, appearing elongated with a relatively smooth light distribution. The central region is brighter and more concentrated, suggestive of a prominent galactic nucleus or bulge. There is evidence of a disk-like structure, although it's not sharply defined and appears somewhat diffuse. The color gradient indicates a higher concentration of bluer stars in the outer regions of the galaxy, potentially indicating ongoing star formation. There are no obvious signs of strong tidal disturbances or major mergers, although some subtle asymmetry hints at possible minor interactions or recent accretion events. The overall appearance suggests a galaxy transitioning between a spiral and elliptical morphology, possibly a lenticular galaxy.
