The galaxy appears to be relatively smooth in morphology, exhibiting a centrally concentrated luminosity profile. It has a generally round appearance, with only a slight deviation towards ellipticity. The dominant color is reddish-orange, suggesting a population of older stars. The presence of some blue tinges on the edges of the galaxy implies the existence of some recent star formation, but this appears to be a minor component compared to the overall stellar population. There is no apparent strong spiral structure or bar. There is no obvious evidence of tidal tails, or any signs of an ongoing major merger. Minor disturbances of the galactic shape appear to be visible in some areas of the galaxy.
