The galaxy presents as a relatively smooth, centrally concentrated object, appearing largely elliptical in shape. The core region exhibits a distinct reddish hue, possibly indicative of an older stellar population. Surrounding the core, a fainter, bluer halo extends outwards, which could signify the presence of younger stars or ongoing star formation. There is a very slight suggestion of a disk-like structure, although the dominant morphology is spheroidal. No signs of active merging or major disturbances are readily apparent, although there is some very slight asymmetry. Overall, the galaxy appears to be an evolved system with a mix of stellar populations.
