The galaxy presents a generally elliptical morphology with a high degree of central concentration. The core region exhibits a bright, yellowish-white hue, suggestive of an older stellar population. There is a smooth decrease in light intensity moving outwards from the core. A faint, diffuse halo surrounds the core, which extends further along the major axis than the minor axis.

There is a slight indication of a possible minor disturbance visible in the lower left portion of the halo, potentially caused by a small interaction. However, the overall structure of the galaxy does not show signs of major disruption. There is no strong evidence of spiral arms or significant star formation regions within the galaxy. Overall, the galaxy appears to be a relatively quiescent system.
