The galaxy presents a generally smooth morphology with a slight elongation, appearing more cigar-shaped than circular. The central region exhibits a concentrated luminosity, suggesting a prominent galactic nucleus or bulge. There is some hint of a disk-like structure. The galaxy displays a color gradient, shifting from a central yellow/orange hue to a slightly bluer tint towards the periphery. There is no obvious evidence of strong spiral arm structure or tidal disturbances to suggest major mergers. The smooth appearance indicates a relatively evolved system, likely an elliptical or lenticular galaxy. The color gradient suggests that there may be some ongoing star formation occurring in the outer regions.
