The galaxy presents a predominantly smooth morphology, with some indication of internal structure. It appears as a flattened spheroid, hinting at a disk component viewed at a relatively low inclination angle. The central region is noticeably brighter, possibly indicating a concentration of older stars or an active galactic nucleus. There's a subtle color gradient, with the central bulge exhibiting a yellowish hue, and the outer regions appearing slightly bluer. This suggests ongoing star formation in the outer disk, although at a modest rate. There are no prominent spiral arms or bar structures visible. There appears to be some minor asymmetry to the galaxy shape indicating perhaps a past minor merger event.
