The galaxy presents as a largely smooth, elliptical structure with a concentrated central bulge. There is a yellow/orange hue in the center, indicative of an older stellar population. The galaxy's overall shape is generally round, with a high degree of symmetry. There is little evidence of spiral arms, dust lanes, or significant star-forming regions within the galaxy. The outskirts appear fuzzier and less defined than the core. The overall impression is that of a relatively quiescent galaxy with minimal current star formation. No signs of mergers or tidal disturbances are apparent.
