The galaxy appears to be an elliptical galaxy, exhibiting a smooth, generally featureless morphology. The light profile suggests a centrally concentrated luminosity, fading gradually towards the outer edges, although not perfectly circular. The galaxy's color suggests that it is likely dominated by an older stellar population. There is a hint of dust or perhaps weak star formation in the central region of the galaxy. No spiral arms or bar structures are discernible. There is no obvious evidence of major interactions or mergers. The light emitted by the galaxy suggests it is not particularly actively forming stars.
