The galaxy appears as a relatively smooth, centrally concentrated object with a diffuse, extended halo. It has a generally elliptical morphology, tending towards round rather than elongated. The central region exhibits a bright, concentrated luminosity profile, suggestive of an older stellar population or perhaps a weak active galactic nucleus, though the resolution is not sufficient to confirm this. There is a hint of a possible tidal interaction or minor disturbance evident by some irregularity in its outer profile, indicating perhaps a recent or ongoing merger event. Colors are suggestive of a mix of stellar populations, but are generally trending toward redder bands.
