The galaxy presents as a relatively smooth, centrally concentrated object, exhibiting a predominantly elliptical morphology. There is very little evidence of spiral arm structures or significant dust lanes, suggesting a classification towards the earlier end of the Hubble sequence.

The galaxy's light profile appears quite uniform, with a gradual decrease in brightness from the core outwards. The color appears consistent with an older stellar population, possibly dominated by redder giant stars. This color may also imply ongoing, but low levels of star formation. There is a possible, faint tidal feature to the lower right, implying a past minor interaction. The overall smoothness points toward an older system that has undergone significant dynamical relaxation.
