The galaxy presents as a somewhat elongated spheroid, potentially viewed at a slight angle. A central, brighter region dominates the galaxy's light profile, exhibiting a yellowish-white hue. This suggests a population of older stars concentrated in the galactic nucleus or bulge. Fainter, bluer emissions extend outwards from the central region, particularly along the major axis of the spheroid. These bluish areas might indicate ongoing, although potentially low-level, star formation within the disk component of the galaxy. The overall structure appears relatively smooth and undisturbed, though slight asymmetries in the outer regions could be hinting at minor gravitational interactions or past disturbances. A potential tidal tail could also be observed on the lower portion of the galaxy, but the resolution is limited. The galaxy appears to be of substantial mass, and its low star formation rate suggests that it may evolve towards a more passive system.
