The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, with a gradual decrease in luminosity moving outward from the center. The galaxy appears mostly uniform in color, presenting a yellowish hue in the central regions. The observed lack of distinct spiral arms or dust lanes suggests a classification towards the elliptical end of the Hubble sequence. There is a faint hint of some bluer regions toward the outer edges of the galaxy. The object exhibits a generally rounded shape. There are no obvious signs of interaction or merging with other galaxies.
