The galaxy presents as a single, concentrated object with a bright central bulge. The overall form appears somewhat elliptical. The luminosity is highest in the central region, decreasing gradually towards the outer edges. There may be an underlying disk, but it is not clearly defined due to the dominance of the central bulge. The color profile suggests the presence of both younger, bluer stars, and older, redder stellar populations. There may be some indication of recent or ongoing star formation. There does not appear to be any clear arm structure or strong signs of dust lanes. There do not seem to be any indications of tidal tails or distortions suggesting the galaxy is not currently undergoing a major merger.
