The galaxy presents as a spiral type, viewed at a slight angle from face-on, though with only a moderate degree of inclination. A prominent central bulge is visible, exhibiting a yellowish-white color indicative of an older stellar population. Extending from the bulge are discernable spiral arms, appearing somewhat patchy. The arms demonstrate a medium winding, wrapping around the central region. The galaxy color suggests a possible ongoing, but perhaps low level, of star formation. The overall appearance is consistent with a galaxy that has experienced some dynamical disturbance or interaction. The structure could be indicative of a mild merger event or gravitational interactions.
