The galaxy presents a predominantly smooth, elliptical morphology, appearing more elongated than perfectly circular. Its light profile exhibits a concentrated central bulge that transitions outward into a less dense, diffuse halo. Color gradients are present, with the core of the galaxy displaying a yellowish-white hue, suggesting an older stellar population. Moving outward from the center, a subtle shift towards redder tones is observed, possibly indicating the presence of dust or a change in the age and metallicity of the stellar population. There is no clear evidence of spiral arms or significant disk features. The galaxy appears relatively undisturbed, lacking any signs of major mergers or significant tidal distortions. There appears to be some minor disturbance in the form of a small blue light region offset from the center. Overall, the galaxy presents the characteristics of a relatively massive, evolved system with low levels of star formation.
