The galaxy presents as a largely elliptical morphology, with a high degree of central concentration. The light profile is smooth and diffuse, indicating a lack of strong spiral arm structure. The primary color is a yellowish-orange hue, suggesting a stellar population dominated by older, redder stars with little ongoing star formation. There is a slight elongation visible, but overall it is mostly round. There is no strong evidence of tidal interactions or significant morphological disturbances, although there may be a hint of some minor disruption on one side.
