This galaxy appears to be a spiral galaxy, viewed at a moderate inclination, though possibly more elliptical. The central bulge is prominent, exhibiting a bright, concentrated luminosity with a yellow to white hue. The disk, while visible, seems relatively smooth with subtle hints of spiral arm structure. A faint blue tinge can be observed within the disk region, suggesting some degree of ongoing star formation. There are no obvious signs of a major merger event, although there is a hint of a possible tidal disturbance. Overall, the galaxy seems to be in a relatively quiescent state.
