The galaxy presents as an elliptical or lenticular system, exhibiting a largely smooth and symmetrical morphology. It displays a concentrated central bulge, grading into a more diffuse halo structure. The color profile suggests an older stellar population, particularly concentrated within the bulge, as indicated by the redder hue. There is a hint of a disk. The system does not appear to be undergoing any major merger events or significant tidal interactions, although there is the possiblity of a minor disturbance. Overall, the galaxy appears to be a relatively undisturbed, evolved system with a moderate mass and limited recent star formation.
