The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish-white hue, suggestive of an older stellar population. Moving outward, the galaxy displays a gradual fading in luminosity and transitions to a redder color profile. This implies a potential gradient in stellar age and composition, with younger, bluer stars possibly being less prevalent in the outer regions. Faint extensions or tidal features are not readily apparent in this image, indicating that major interactions or mergers are unlikely to be actively deforming its structure at this resolution. The galaxy appears relatively undisturbed and isolated within the observed field.
