The galaxy presents a largely smooth morphology, with a high degree of circularity. There is a notable central bulge that appears yellow-white, suggesting an older stellar population. A faint disk-like structure is observed surrounding the bulge, displaying some faint arms, but lacking well-defined spiral structure. There is some indication of potential minor disturbance in the outer regions, but no major merging event seems to be in progress. The redder hue in the surrounding areas suggest some ongoing star formation.
