The galaxy presents as a single, centrally concentrated object, appearing generally smooth with a high degree of roundness. It exhibits a dominant yellow-orange hue, suggesting a population of older stars. There is a possible secondary concentration below the central part that is very slightly more red. The lack of distinct spiral arms or significant dust lanes suggests a classification towards the elliptical end of the Hubble sequence. Despite its overall smoothness, subtle disturbances in the light distribution suggest the possibility of ongoing or past minor merger events. Overall, it shows signs of being a fairly massive galaxy, based on the luminosity, with a relatively low current star formation rate.
