The galaxy presents a somewhat lenticular morphology, exhibiting a prominent central bulge that gradually fades into a diffuse, extended disk. There are no clearly defined spiral arms or strong bar features visible, which is consistent with this type of galaxy. The color distribution suggests a relatively older stellar population, given the subtle reddish hue, although there are hints of bluer regions, particularly in the outer disk, indicating the presence of some younger, hotter stars. The overall structure appears relatively undisturbed, without any obvious signs of a major merger or significant tidal interactions. The galaxy is estimated to have a moderate mass, with a corresponding moderate rate of star formation.
