The galaxy presents as a relatively smooth, elongated structure. The central region exhibits a concentrated, bright core that appears yellowish-white, indicating an older stellar population. Fainter, bluish light is present in the outer regions, suggesting the presence of younger stars and possibly ongoing star formation, though the rates appear moderate. The overall shape is somewhat cigar-shaped, with a noticeable lack of spiral arm structure. There are hints of minor disturbances in the galaxy's morphology, though no major merging events or strong tidal features are apparent. The galaxy's light distribution is fairly even, with a gradual decrease in intensity from the center outwards.
