The galaxy presents as a relatively smooth, elliptical form with a bright, concentrated central bulge. The light distribution suggests it is largely spheroidal. A slight elongation is observed, with the apparent shape falling between round and cigar-shaped. The galaxy exhibits a color gradient, transitioning from a bluer hue in the outer regions to a redder hue in the core, implying possible differences in stellar populations. The outer regions appear somewhat diffuse and lack distinct structural features. There's no obvious evidence of spiral arms or a prominent disk. Furthermore, there are no clear signs of any ongoing major merging activity or significant tidal disturbances, though a minor disturbance cannot be ruled out. Overall, the galaxy appears to be relatively evolved and quiescent.
