The galaxy presents as a spiral type, displaying well-defined spiral arms. The arms are prominent and exhibit a moderately wound structure. The presence of a central bulge is apparent, contributing a significant portion to the overall luminosity of the galaxy. A bar-like structure can not be fully determined. The overall color of the galaxy suggests an actively star-forming population, particularly within the spiral arms. No signs of major mergers or significant tidal disturbances are visibly apparent, although a slight distortion may be present.
