The galaxy appears as a centrally concentrated object, with a morphology that is primarily smooth. Its overall shape is somewhat elliptical, but tending towards round. There is little evidence of strong spiral arm structures or prominent features, but there is subtle disking. A color gradient is observed, with the central regions appearing more yellowish, potentially indicating an older stellar population or higher dust content. The outer regions appear slightly bluer, suggesting the possibility of recent star formation activity at the periphery. The galaxy does not seem to be undergoing any major mergers, though there may be very slight disturbances in its shape. Overall, the light profile appears relatively regular and undisturbed.
