The galaxy presents an elliptical morphology, appearing largely smooth and lacking distinct spiral arm structures. Its overall shape is fairly round, with a slight deviation toward an elongated form. The light distribution suggests a centrally concentrated brightness profile, with the intensity gradually diminishing towards the outer regions.

There is a notable color gradient across the galaxy. The central region exhibits a yellowish-white hue, possibly indicating the presence of an older stellar population. Surrounding this core, a bluish halo extends outwards, which may signify the presence of younger, hotter stars. Some disturbances in the shape indicate that the galaxy may have been involved in a minor merger. The galaxy appears relatively compact, suggesting a moderate physical size for its type.
