The galaxy presents as a relatively compact, somewhat elliptical object. The light distribution appears mostly smooth, lacking any distinct spiral arm structures or prominent dust lanes. The galaxy exhibits a central concentration of light, suggesting a bulge component. The color profile indicates a bias towards shorter wavelengths, with a bluish hue permeating the galaxy. There may be a slight asymmetry in the outer regions, but its overall form is largely undisturbed, showing no signs of a major ongoing merger. Overall, it appears to be a spheroidal galaxy with ongoing star formation.
