The galaxy appears as a relatively compact, elliptical-like structure. It exhibits a smooth, largely featureless morphology, with no prominent spiral arms or a distinct disk component visible in this image. The primary color of the galaxy is a pale blue-white, suggesting the presence of a population of younger, hotter stars, however, the overall lack of distinct features suggests that star formation is not occurring at a high rate. The galaxy is moderately luminous, and appears to be fairly massive. There is no evidence of ongoing major merger activity or significant tidal disturbances. The galaxy appears relatively isolated in the image field.
