The galaxy presents as a somewhat smooth, centrally concentrated structure. The core region exhibits a yellowish hue, suggesting an older stellar population. A slightly fainter, more diffuse halo surrounds the core. There are hints of a disclike morphology, but no defined spiral arm structures are visible. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or significant tidal interactions, although minor disturbances cannot be ruled out. There appears to be a low rate of star formation. Overall, the galaxy seems to be an intermediate type, possibly tending towards a lenticular classification.
