The galaxy presents as a relatively compact, elliptical-like structure. The light distribution appears centrally concentrated, with a smooth and diffuse profile. The core exhibits a yellowish-white hue, suggesting a population of older stars. The overall color gradient shows a slight reddening towards the outer regions. There are no obvious spiral arm features or dust lanes visible, indicating a lack of significant ongoing star formation. The shape is moderately rounded, and no significant tidal features or signs of major mergers are apparent. Faint disturbances or asymmetry may be present within the galaxy.
