The galaxy appears to be an elliptical type, characterized by a smooth, relatively featureless morphology. The light distribution is centrally concentrated, with a diffuse, gradual decline in brightness towards the outer regions. There is little evidence of spiral arm structure or significant dust lanes. The galaxy exhibits a yellowish-white hue, indicating an older stellar population with fewer young, massive stars. Its overall shape appears close to round with a slight deviation and some elongation, and does not show obvious signs of ongoing major mergers or significant tidal disturbances. Based on the color and smooth appearance, it could be undergoing low star formation.
