The galaxy presents a largely smooth and rounded morphology, with a high degree of central concentration. The galaxy core exhibits a bright, diffuse glow, indicative of a high stellar density and potentially an active galactic nucleus. Moving outwards from the core, the luminosity gradually decreases. There is only some evidence of a disklike structure, as well as some hints of faint spiral arms or dust lanes, but these features are not sharply defined. The overall color appears somewhat red, suggesting a population of older stars. There appears to be little evidence of ongoing major star formation. No significant tidal disturbances or merging features are readily apparent.
