The galaxy appears to be an elliptical type, exhibiting a smooth, centrally concentrated light distribution with no discernible spiral arms or dust lanes. It presents an overall diffuse, somewhat rounded morphology, with a slight elongation. The color is predominantly yellowish-white, suggesting an older stellar population with relatively low levels of ongoing star formation. There is no obvious evidence of any major mergers or significant tidal disturbances affecting its structure, though a possible minor asymmetry is present, which may be indicative of past interactions. The galaxy's estimated size and luminosity indicates a substantial stellar mass.
