The galaxy presents as a relatively small, elliptical shape on the sky. Its central region exhibits a bright, concentrated core, suggestive of a substantial galactic nucleus. Peripherally, a fainter, diffuse halo extends outwards, diminishing in intensity with distance from the core. Within the disk structure, some apparent disturbances are observed. These include a faint, asymmetrical arm-like structures extending from the main body. Overall, the light distribution appears relatively smooth, but with some features within the central area. Color gradients are observed, with the core exhibiting bluer tones compared to the more reddish halo.
