The galaxy presents a morphology that is neither purely elliptical nor spiral, appearing as a disk galaxy but with an indistinct spiral arm structure. The central bulge is prominent and exhibits a yellowish hue, suggestive of an older stellar population. Moving outward from the center, there is a diffuse disk with a slightly bluish tint. This indicates the presence of ongoing star formation and younger, hotter stars. There are some indications of a possible tidal disturbance, with the main body of the galaxy appearing slightly elongated and irregular. A mild interaction with other objects can not be ruled out.
