The galaxy appears as a relatively smooth, elliptical-like structure with a concentrated central bulge. The overall color profile is yellowish, suggesting a population of older stars with suppressed star formation. The isophotes are generally elliptical, but with some subtle deviations from perfect symmetry. There is no clear indication of spiral arms or a prominent disk. The galaxy appears relatively isolated, without obvious signs of major interactions or mergers. There might be a hint of a very faint tidal tail or minor disturbance in the immediate vicinity.
