The galaxy presents as an elliptical or lenticular morphology, exhibiting a smooth, diffuse light distribution. The core region is markedly brighter and appears yellowish, suggesting a concentration of older stellar populations. The galaxy's shape is elongated, approximately cigar-shaped, with a noticeable tilt relative to the line of sight. The outer regions show a gradual fading of light intensity. There is a hint of a disk component, but it is not well-defined. There may be some evidence of minor disturbances in the outer regions, possibly indicative of past interactions, but the overall structure appears relatively undisturbed.
