The galaxy presents as a centrally concentrated object, exhibiting a generally smooth morphology. The light profile indicates a spheroidal structure with no apparent spiral arms or bar features. The core region appears more luminous and exhibits a yellowish-orange hue, suggesting an older stellar population. The outer regions appear fainter and slightly more diffuse. There may be some minor disturbances, but the overall structure does not indicate a recent major merger event. The shape is largely round with only slight deviations. Star formation appears to be largely suppressed.
