The galaxy presents an overall elliptical morphology with a noticeable bulge component. The color is predominantly yellow and orange, suggesting a stellar population that is generally older and redder. There may be a slight disk component present; the lack of distinct spiral arms would indicate that the galaxy is a lenticular or early-type spiral galaxy.

The central bulge appears smooth and concentrated, indicative of a significant population of older stars. The color temperature shifts from a hot inner core to a cooler halo of stars in the outer edges of the galaxy. A slight elongation is noticeable, leaning towards a cigar shape. Overall, the galaxy appears relatively undisturbed and isolated, without any obvious signs of major mergers or tidal interactions.
