The galaxy appears as a moderately luminous object, elongated in shape with an approximate estimated radius of 5.4 kpc. Its overall morphology suggests it is likely an elliptical galaxy.

The color distribution indicates a concentrated, yellowish core region which gradually fades into a more diffuse reddish halo. This color gradient may be indicative of variations in stellar populations or dust content, with potentially older, redder stars dominating the outer regions and possibly ongoing star formation in the interior. The galaxy exhibits a smooth texture, suggesting a lack of significant spiral arm structures or major dust lanes. There is no readily apparent evidence of a major merger event or significant tidal disturbances in its immediate vicinity, though minor disturbances cannot be ruled out. The observed shape suggests some degree of rotational support, or perhaps a triaxial structure.
