The galaxy presents as an elliptical morphology, exhibiting a centrally concentrated light profile. The core region shows a yellowish-white hue, likely indicating an older stellar population and a lower rate of star formation. Moving outwards from the center, the color transitions to a slightly bluer tone, suggesting a small amount of younger stars toward the outer regions. The overall shape of the galaxy is slightly elongated with the degree of roundness appearing to be of an intermediate nature. There are no clear signs of spiral arms or significant dust lanes. The overall structure appears relatively smooth and undisturbed, showing no visual evidence of a major merger event, with only hints of potential minor disturbance.
