The galaxy exhibits a predominantly red hue, suggesting a population of older stars, or significant dust obscuration. The object appears relatively compact, with an estimated effective radius on the order of a few arcseconds. There is a faint, diffuse structure that may indicate tidal disturbances or recent interactions, however, this is very minor. The primary body of the galaxy is generally smooth in appearance, with no prominent spiral arms or bar structure readily discernible. There appears to be only a very slight indication of a disk. The galaxy is relatively isolated, lacking any bright nearby companions that might suggest an ongoing merger event.
