The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. It exhibits a nearly circular shape with a faint extended halo. The color profile suggests a dominant population of older stars, giving it a yellowish hue. There is no indication of spiral arm structure or active star forming regions. There are no signs of tidal debris or significant morphological disturbances indicative of ongoing or recent major merger events. The galaxy's smooth profile and color are consistent with an elliptical or lenticular classification.
