The galaxy appears as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution is fairly uniform, with no distinct spiral arms or strong dust lanes visible. The galaxy exhibits a yellowish-orange hue, suggesting a dominant population of older stars and a relatively low rate of ongoing star formation. There is a slight elongation, but the galaxy is largely circular in appearance. No signs of major disturbances or interactions with other galaxies are readily apparent, although minor disturbances cannot be ruled out given the image resolution.
