The galaxy presents as an elliptical morphology with a smooth, centralized light distribution. It appears nearly round in shape. There is a slight color gradient; the central region seems to exhibit a yellower hue, which could indicate an older stellar population. The outer regions appear slightly bluer, which suggests the presence of younger stars and possibly ongoing star formation. No distinct spiral arms or bar structures are visible. There appear to be no signs of major interaction or merging events. The overall impression is of a galaxy in a relatively quiescent state.
