The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing largely spheroidal in shape with only a slight deviation from perfect circularity. The color profile indicates a dominance of older stellar populations, with a yellowish-red hue concentrated towards the core. This suggests ongoing star formation at a moderate rate. There is no evidence of distinct spiral arm structures or a prominent disk. Minor irregularities are present, but there is little to no evidence of any major merger or interaction with another galaxy. The galaxy is somewhat compact, with light tapering gradually from the core towards its outer regions.
