The galaxy presents a primarily smooth morphology, with a largely elliptical appearance. There is a slight disk like feature with very faint spiral structure. The color profile suggests an older stellar population, with a redder central bulge surrounded by a bluer halo region. Evident minor disturbances suggest possible interactions or recent minor mergers. The galaxy is relatively compact, with an estimated effective radius of roughly 9 kpc. Overall, this galaxy appears to be an early-type spiral with low ongoing star formation.
