This galaxy presents as a spiral structure, with a notable central bulge that appears moderately sized. The arms appear somewhat tightly wound and are not as clearly defined, giving the galaxy a more diffuse appearance. There is a slight asymmetry evident in the spiral arm structure suggesting some sort of interaction or disturbance. The galaxy has a relatively high surface brightness in the central regions, indicative of a higher stellar density and potentially a more actively star-forming region or a significant older stellar population. The overall color profile suggests the presence of both older stars in the central bulge and younger stars distributed throughout the arms. No strong bar structure is immediately apparent.
