The galaxy presents as a largely smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing more oblate than prolate in shape. A bright, yellowish core dominates the central region, suggesting a significant population of older stars. The color of the core light suggests it contains a large population of evolved stars with relatively low star formation. There are no signs of significant tidal features or ongoing major mergers. Faint, diffuse light extends outwards from the central region, gradually fading into the background. The light extending outwards also displays a similar yellowish hue, suggesting a homogenous population of evolved stars throughout the galaxy. There is no presence of spiral arms or any other significant features.
