The galaxy presents as a spiral type, with a prominent central bulge that appears moderately sized. Evident spiral arms extend outwards from the bulge, displaying a somewhat flocculent structure. There is a hint of active star formation within these arms, indicated by the presence of bluer regions. However, the overall color suggests a relatively older stellar population, with regions of yellow and red light present. The galaxy appears relatively undisturbed, showing no significant signs of a major merger event. There's a possible, slight disturbance on the outer edges of the disk. A weak bar structure may be present, but not clearly defined. The galaxy's disk is presented face-on.
