The galaxy presents as a generally smooth, elliptical object. It exhibits a concentrated central bulge that appears nearly spherical. The light profile suggests a gradual decrease in luminosity from the core outwards. The galaxy displays a slight bluish tint, especially in the central region, potentially indicating the presence of younger, hotter stars. No distinct spiral arms or prominent dust lanes are immediately visible. There is also a notable absence of strong tidal features or significant distortions in the galaxy's shape suggesting it has not undergone a major merger recently. Close inspection suggests a minor disturbance in shape, though the light distribution is still largely spheroidal. Overall, the galaxy's morphology points towards it being an elliptical galaxy with some features of a disc galaxy and relatively low ongoing star formation.
