The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge that transitions smoothly into a fainter, diffuse halo. The galaxy appears largely spheroidal in shape, with no distinct spiral arm features visible. There is a slight elongation, suggesting it is not perfectly spherical. Color gradients suggest a redder core, potentially indicative of an older stellar population, while bluer hues are observed in the outer regions, possibly suggesting recent star formation. No significant dust lanes or prominent features of ongoing mergers are discernible. Overall, the galaxy's morphology is characteristic of an evolved elliptical galaxy.
