The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing largely round in projection. There is little evidence of significant spiral arm structure or prominent dust lanes. The light profile suggests a concentration of older stellar populations towards the core, with a gradual decrease in surface brightness outwards. The galaxy does not appear to be undergoing any major merging events or displaying significant tidal disturbances. There is no indication of a bright, active galactic nucleus. The overall color is consistent with a population of primarily older stars, suggesting a relatively low current star formation rate.
