The galaxy presents as a relatively smooth, centrally concentrated structure with a flattened, elliptical morphology. A noticeable bulge is observed at the galaxy's center, exhibiting a yellowish hue, potentially indicating an older stellar population and lower rates of star formation in this region. The outer regions show a gradual decrease in surface brightness, and appear more irregular in shape. Some faint bluish tones can be seen in the outer regions, which might suggest some presence of younger, hotter stars and ongoing star formation there, though at a low level. Overall, the galaxy's structure appears relatively undisturbed, lacking any major signs of tidal interactions or ongoing mergers. The galaxy's overall color suggests an intermediate stellar population, somewhere between a typical early-type and late-type galaxy.
