The galaxy presents a generally smooth morphology, appearing elliptical in shape, with a discernible elongated structure. A central bulge is prominent, exhibiting a yellowish-orange hue, suggesting an older stellar population. Diffuse, fainter light extends from the central region, with some hints of bluer colors on the edges, which could potentially indicate some regions of ongoing star formation. Faint disturbances can be observed, suggesting a possible interaction or minor merger event in its past. The overall color profile indicates that the bulk of the stellar population is relatively old, though there are small signs of some young stars being created. The galaxy appears to be in a relatively evolved state.
