The galaxy presents a generally smooth and concentrated appearance. It exhibits a centrally concentrated bulge, which appears largely spheroidal and dominates the overall light profile. Fainter light extends outwards from the central bulge, with little evidence of a significant disk component. The overall color profile suggests a population of older stars, with the central region appearing more yellowish than the outer regions, which tend towards red. The galaxy shows no obvious signs of significant tidal disturbances or interactions with other galaxies, nor any pronounced spiral arm structures or features. The shape is primarily round, with minor deviations from perfect circularity. Overall, the galaxy appears to be a relatively undisturbed, evolved system with limited ongoing star formation.
