The galaxy presents a predominantly smooth morphology, appearing as a diffuse, elliptical structure with a concentrated central region. Color gradients suggest a possible variation in stellar populations, with the core exhibiting a yellowish hue, potentially indicative of older, redder stars. There are hints of a slightly elongated shape, though it is close to round. No distinct spiral arms or prominent dust lanes are discernible. The galaxy shows signs of disturbance and merger, possibly due to tidal interactions with smaller companion galaxies or past mergers. The light distribution appears relatively uniform, lacking strong features. The overall color is consistent with that of a mature galaxy with a moderate rate of star formation.
