The galaxy presents as a roughly elliptical structure with a bright, concentrated central bulge that emits strongly in yellow-white light. The outer regions of the galaxy are less defined, appearing more diffuse and extending outwards in a flattened disk-like fashion. These areas show a slight reddening effect. There is no obvious spiral arm structure visible; the morphology appears smooth, with subtle hints of disturbances in the outer edges. The color profile suggests a relatively evolved stellar population, potentially with ongoing, albeit relatively low levels of star formation activity. Overall, the galaxy exhibits characteristics of a late-type spiral galaxy undergoing transition to a more elliptical morphology. The central bulge appears prominent and relatively massive compared to the surrounding disk. There may be minor interactions occurring which cause disturbance in the outer regions.
