The galaxy presents a generally smooth, elliptical morphology. The light is concentrated towards the center, with a bright, yellowish core that may indicate an older stellar population or the presence of an active galactic nucleus, though the resolution is insufficient to determine this with certainty. Diffuse, fainter light extends outwards, exhibiting a slightly flattened profile suggestive of a disk component, although this is not strongly pronounced. There are subtle color gradients, shifting from yellowish-white in the center to slightly redder hues in the outer regions. There is no clear indication of spiral arms or significant dust lanes within the galaxy's structure. The overall appearance indicates a mature system with a significant fraction of older stars and limited ongoing star formation activity. There does not appear to be any sign of galactic merging or major disturbances.
