The galaxy appears to be a relatively small, early-type galaxy, exhibiting a smooth, elliptical morphology. Its light profile suggests a centrally concentrated spheroid. There are no discernable spiral arms or a distinct disk component. The galaxy's color is predominantly blue, hinting at the presence of at least some young, hot stars, but the overall smooth appearance suggests that star formation has been subdued or is occurring at a low rate. There are no signs of any major ongoing mergers, but subtle features are visible that suggest the possibility of minor past interactions or disturbances, such as a slight asymmetry in its light distribution.
