The galaxy presents as a centrally concentrated, smooth object with a predominantly elliptical morphology. The light distribution appears largely homogenous without any discernible spiral arms or significant dust lanes. The color is predominantly yellow-white, suggesting an older stellar population with fewer young, hot stars. There is a slight color gradient, with the central region appearing somewhat more yellow, possibly indicating a higher concentration of older stars towards the core. The galaxy exhibits a relatively high degree of circular symmetry in its overall shape. There is no obvious evidence of any ongoing major merger events or significant tidal disturbances. The overall appearance suggests a relatively evolved system that is quiescent in terms of star formation. A very faint extension or halo is vaguely visible around the object.
