The galaxy presents a primarily smooth, elliptical morphology. It displays a concentrated central bulge that appears nearly spherical. The galaxy's color profile indicates a relatively older stellar population, with a subtle shift towards redder hues compared to bluer star-forming regions. There is a faint disk-like structure that is nearly face-on and is tilted slightly. No apparent spiral arm structures, dust lanes, or strong signs of active star formation are visible. The galaxy's outskirts fade gradually into the background sky, suggesting a large but diffuse halo. There may be some minor disturbances present within the galaxy's structure, but they are not prominent in this image. Overall, the galaxy appears to be a relatively evolved and quiescent system.
