The galaxy presents an elliptical morphology, exhibiting a smooth, featureless structure with no discernible spiral arms or bar. A bright, concentrated central bulge dominates the galaxy's core, surrounded by a more diffuse halo of starlight that gradually fades into the background. The galaxy appears somewhat rounded, with a slight elongation suggesting it is not perfectly spherical. There is no obvious evidence of ongoing major mergers or significant tidal disturbances in its immediate vicinity. Subtle color gradients can be observed, with the core appearing slightly bluer compared to the outer regions, possibly indicating a moderate level of recent or ongoing star formation.
