The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The light distribution suggests a spheroidal shape, with a gradual decrease in brightness from the core outwards. There's a hint of disk-like structure but no clear spiral arms are visible. The color profile indicates a predominantly older stellar population, with a yellowish hue in the central region transitioning to slightly bluer colors in the outer regions, likely due to some recent star formation. There is no evidence of significant tidal disturbances or ongoing mergers; the galaxy appears relatively undisturbed. The galaxy has an estimated half-light radius of approximately 6.5 kpc.