The galaxy appears to be a relatively smooth, elliptical or lenticular type. Its light profile indicates a centrally concentrated spheroid with a gradual decrease in surface brightness moving outwards. The core region exhibits a yellow-white hue, suggesting an older stellar population. The lack of distinct spiral arm structures or prominent dust lanes is notable. Overall, the galaxy appears relatively undisturbed, showing no obvious signs of recent major mergers or interactions, though there is a minor possibility of disturbance. Given the observed morphology and color profile, it seems likely to be a massive system with a low star-formation rate.
