The galaxy appears as a somewhat elliptical structure with a bright, concentrated central bulge. The bulge exhibits a yellowish-orange hue, suggesting an older stellar population. Fainter, bluer light is visible extending away from the central region, possibly indicative of younger stars or regions of ongoing star formation within a disk component. The galaxy does not display strong spiral arm features, and its overall structure appears relatively smooth. There is a slight asymmetry in the outer regions, which could point to a minor gravitational disturbance or interaction with another galaxy.
