The galaxy presents a generally smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, appearing brightest toward the core and gradually diminishing outwards. The color profile suggests a population of older stars, with a redder hue dominating the galaxy's overall appearance. There is very little evidence of spiral arm structure. The galaxy shows a slight elongation, appearing to be somewhere between round and cigar-shaped. There is some visual evidence of minor disturbances, potentially indicative of past interactions or mergers. The overall impression is that of a relatively massive galaxy with a suppressed rate of star formation.