The galaxy exhibits a generally smooth morphology, but also shows evidence of disk-like structure. The central bulge appears prominent and exhibits a yellowish hue, indicative of an older stellar population. Fainter, bluer extensions are visible emerging from the central region, suggesting the presence of younger, star-forming regions within a disk. The overall shape is somewhat elongated. There is a possible minor asymmetry or disturbance in the outer regions of the galaxy, suggesting potential past interactions or mergers.
