The galaxy presents as a moderately bright, elliptical-like structure, exhibiting a smooth and relatively featureless morphology. A substantial central bulge region dominates the light profile, appearing more concentrated and yellow-white in color, suggesting an older stellar population. Fainter, more diffuse light extends outward from the central bulge, creating a somewhat elongated shape. The outer regions are less distinct and appear to fade gradually into the background. There is some evidence of a subtle disk component oriented roughly along the major axis of the galaxy, showing very faint bluish tones indicating the presence of younger stars. Overall, the galaxy's smooth appearance suggests that it is a relatively evolved system. There is no strong evidence of active star formation or significant dust lanes. The color gradient indicates a gradual shift from older stars in the center to more recent star formation on the outside of the disk.
