The galaxy presents a morphology that is largely smooth, but exhibits some irregular features and a suggestion of a disk component. It has an intermediate degree of roundness, neither perfectly spherical nor highly elongated. There may be some evidence of minor tidal disturbances or interaction with other objects, or perhaps an ongoing merger event. The central region exhibits a concentration of light, fading towards the edges. The color profile suggests a mix of stellar populations, with a bluer component in some regions, indicating areas of recent or ongoing star formation. The overall color appears somewhat redder, suggesting a dominant population of older stars and a relatively low star formation rate.