The galaxy presents a relatively smooth, elliptical morphology. Its central bulge is prominent and exhibits a bright, concentrated luminosity, suggesting a high density of stars. The color of the central region appears yellowish-white, potentially indicating an older stellar population. Extending outward from the bulge, the galaxy displays a diffuse halo. There is very little evidence of defined spiral arms or significant dust lanes. The overall color becomes slightly redder with increasing distance from the center. A lack of distinct blue regions suggests a relatively low current star formation rate. The galaxy is elongated in shape, with no visible signs of interactions or major disturbances.
