The galaxy presents as a somewhat smooth, elliptical-like structure with an overall shape that appears moderately rounded. Its core region exhibits a bright, concentrated luminosity, with a gradient decrease in intensity extending outwards. There appears to be a tidal tail or perhaps an interacting companion galaxy on one side. The light from the galaxy is primarily whitish-blue, possibly suggestive of moderate recent star formation. However, the presence of some reddish hues mixed in indicates an older stellar population, possibly in the bulge. This suggests that the galaxy is actively forming stars, but is not exclusively blue due to an already mature population. The galaxy does not show any strong evidence of a spiral arm structure.
