The galaxy presents as a moderately luminous system exhibiting a relatively smooth morphology with some discernible features. Its overall shape appears elongated, potentially exhibiting a disk-like structure viewed at an angle. The central region displays a concentration of light, possibly indicating the presence of a bulge. 

The galaxy’s color is predominantly yellowish, suggesting a stellar population that is somewhat older, with ongoing but modest star formation. There are hints of subtle disturbances or irregularities in the outer regions, which might be indicative of minor tidal interactions or past merger events. Some faint, extended features can be observed around the main body of the galaxy, implying a diffuse halo or the presence of stellar streams.
