This galaxy appears to be a spiral galaxy viewed at a moderate inclination. It presents a bright, concentrated central bulge which is yellowish in color, suggestive of an older stellar population. A faint disk is visible around the bulge, with hints of spiral structure. The disk appears somewhat disturbed, possibly exhibiting minor tidal features. There are some areas of bluer light distributed in the disk, indicating regions of more recent star formation, but overall, it appears to be a galaxy undergoing a lower rate of star formation, as evidenced by the bulge color. There is no clear indication of a recent major merger event, although some minor gravitational interaction cannot be ruled out based on the subtle disk asymmetry.
