The galaxy presents as a relatively smooth, centrally concentrated object, likely an elliptical or lenticular galaxy based on its morphology. It exhibits an oblate spheroidal shape, appearing mostly round with a slight elongation. There is no obvious spiral arm structure or significant dust lane features visible. The color gradient suggests an older stellar population, with a yellowish-red hue indicative of evolved stars. No strong signs of active star formation are immediately apparent in the galaxy's overall color. There is some minor evidence of a slight disturbance.