The galaxy presents as a somewhat elliptical form, appearing predominantly smooth in structure with a notable central bulge. A faint, diffuse disk is perceptible extending outward from the core. Color gradients suggest a higher concentration of older stellar populations in the central region, indicated by the yellowish hue. The outer regions of the disk exhibit a bluer tint, hinting at more recent star formation activity. There are no prominent spiral arms or bar structures visible. The galaxy's overall morphology is largely undisturbed, with no evident signs of major tidal interactions or ongoing mergers. A slight asymmetry is present in the outer disk.
