The galaxy presents a relatively smooth, elliptical morphology. The central region is dominated by a bright, concentrated bulge exhibiting a yellowish-orange hue, indicative of an older stellar population. The galaxy appears to be relatively isolated, without any obvious major mergers or tidal disturbances. The outer regions of the galaxy fade gradually, showing hints of a disk-like structure. A redder patch is located on the edges, suggesting regions of ongoing, but diminishing star formation. Overall, this galaxy appears to be an intermediate-mass elliptical galaxy with little to no active star formation.
