The galaxy appears as a relatively smooth, centrally concentrated object with a predominantly elliptical morphology. The light distribution is concentrated towards the center with a fairly rapid drop-off in intensity outwards from the core, consistent with an early-type galaxy, perhaps an elliptical or lenticular system. There is little evidence of spiral arm structure or prominent dust lanes. The core exhibits a yellow-red hue, suggesting a population of older stars. The outer regions appear slightly bluer, indicative of younger stellar populations or ongoing star formation, albeit at a low level. There appears to be some minor tidal disturbance, perhaps indicating a prior minor merger event or ongoing gravitational interaction with a nearby companion.
