The galaxy presents as a primarily smooth, elliptical structure. The core is a bright, concentrated region, exhibiting a yellowish hue that suggests an older stellar population. The surrounding halo displays a gradual decrease in luminosity, fading into the background sky. There is a subtle extension along one axis, indicating a slight cigar shape rather than a perfect sphere. No distinct dust lanes or spiral arm structures are discernible, supporting the classification as an elliptical galaxy. There is no apparent evidence of any major merging events or significant tidal disturbances. The galaxy seems to be an isolated system in a relatively undisturbed state.
