The galaxy presents as a centrally concentrated object with a smooth, diffuse appearance. The core exhibits a yellowish-white hue, possibly indicating an older stellar population. The galaxy's outer regions display a faint bluish tint, suggesting the presence of some younger, hotter stars, although star formation appears relatively quiescent. The galaxy displays a slightly elliptical morphology, with the ratio of its major to minor axes indicating a moderate degree of flattening. There is no clear evidence of spiral arm structures or other prominent features such as dust lanes or active galactic nuclei. The overall impression is that of a relatively evolved galaxy, possibly an early-type spiral or elliptical galaxy. No signs of major tidal disturbances or ongoing mergers are apparent.
