The galaxy appears to be a relatively compact object, likely an elliptical or lenticular type, based on its generally smooth and rounded morphology. The light distribution suggests a centrally concentrated structure with a gradual decrease in brightness outwards. There is a hint of a slightly elongated shape, but it's mostly circular. The color profile suggests the presence of older stellar populations, indicated by the redder hue. There are no distinct spiral arms or prominent dust lanes visible, further supporting a classification as an early-type galaxy. There is no obvious evidence of any major mergers or significant tidal disturbances in the immediate vicinity.