The galaxy exhibits a centrally concentrated light distribution, appearing generally smooth in morphology. The overall shape is elongated, deviating from a perfectly circular form. A faint, diffuse halo appears to surround the central region, extending a short distance from the main body of the galaxy. There is no obvious spiral structure, nor are there prominent dust lanes or tidal tails. Close inspection reveals hints of subtle internal structures, such as minor fluctuations in brightness. There is little to no evidence of recent or ongoing major mergers or interactions with other galaxies.
