The galaxy presents as a relatively smooth, elliptical-like object with a high degree of central concentration. There is a slight elongation apparent in the shape, suggesting it is not perfectly spherical, with a hint of a cigar-shaped morphology. The color profile indicates a higher presence of older stellar populations, emitting a yellowish-red hue, concentrated mainly in the core, which implies a ceased or very low ongoing star formation rate. Subtle color variations within the galaxy suggest some minor internal structure. No prominent tidal features, or signatures of major interactions or mergers are evident, although there is a possibility of minor gravitational disturbance.
