The galaxy presents as a moderately bright, elliptical-like structure. It appears largely smooth with a notable central bulge. There is a slight elongation, suggesting a deviation from perfect sphericity; closer to a flattened spheroid shape. The core exhibits a concentrated yellowish to orange hue, which implies a population of older stars. Surrounding the core is a more diffuse and subtle greenish halo. There is no obvious evidence of spiral arms, dust lanes, or significant tidal disturbances. There is no strong indication of active star formation or recent merging activity based on its shape. Overall, the galaxy appears to be a relatively quiescent system.
