The galaxy presents as an elliptical morphology, although there may be some disk-like components present. It exhibits a generally smooth appearance, with minimal apparent features such as spiral arms or distinct dust lanes. The central region shows a bright, concentrated bulge, surrounded by a more diffuse halo of light. The overall color profile suggests a population of older stars, with a trend towards redder wavelengths, particularly concentrated in the central bulge. There is a possibility of minor gravitational interactions. The galaxy appears to be a relatively undisturbed system.
