The galaxy presents a generally smooth morphology, with a notable central bulge exhibiting a bright, concentrated luminosity. The galaxy appears to be largely elliptical in shape, tending toward round. There are potential signs of a minor disturbance, with a feature to the side of the galaxy displaying a warmer color. This could be indicative of a potential minor merger or tidal interaction. The overall color profile suggests a well-evolved stellar population, although the bluer color hints at some ongoing, albeit subdued, star formation. The galaxy's intermediate redshift suggests a considerable distance.
