The galaxy presents an elliptical morphology, appearing as a smooth, centrally concentrated spheroid with a notable lack of discernible spiral arms or disk-like features. The object exhibits a slight elongation, with an axis ratio deviating marginally from a perfect circle. Color gradients within the galaxy suggest a redder core, potentially indicating an older stellar population or higher dust concentration towards the center. The outer regions appear bluer, possibly signifying the presence of younger, hotter stars, although this is subtle. There appears to be minor asymmetry in the outer regions, suggesting possible minor tidal disturbances or interactions. Overall, the galaxy presents an early-type morphology, and low to medium levels of star formation, typical of this galaxy type.
