The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge, visually dominating the galaxy's structure. The luminosity profile appears to decrease steadily from the center outwards. The color gradient suggests an aging stellar population, with the central regions exhibiting a yellowish hue, potentially indicating a higher concentration of older stars. The outer regions appear slightly bluer, which could suggest the presence of younger stars, though star formation appears generally quiescent. There is no clear evidence of spiral arms, a central bar, or significant tidal disturbances indicative of recent major mergers. The galaxy’s overall shape appears somewhat elongated, but generally well-formed.
