The galaxy presents as an elliptical shape, appearing relatively smooth in texture. There is a distinct central bulge, exhibiting a concentrated brightness that declines gradually towards the edges. A faint, diffuse halo surrounds the core, with no clearly defined spiral arms or substructures. The color profile suggests a population of older stars, with a relatively high red color index and a lower blue color index, implying a lower rate of ongoing star formation. There is a subtle hint of distortion in the overall shape, possibly indicative of minor gravitational interactions or past mergers. The light distribution appears mostly uniform, lacking prominent dust lanes or star-forming regions.
