The galaxy appears as a relatively smooth, elliptical-like structure. It exhibits a concentration of light towards the center, indicative of a bulge. The galaxy displays a dominant red hue, with some evidence of bluer regions primarily in the outer parts, which suggests the presence of some star formation but is mainly composed of an older stellar population. There are no clear signs of spiral arms or a prominent disk-like structure and no significant morphological disturbances. It seems to be an isolated galaxy, with no obvious signs of interaction with other galaxies. The galaxy is somewhat compact and shows a fuzzy, indistinct edge.
