The galaxy presents as a slightly elliptical, luminous object with a smooth, diffuse structure. The central region is brighter, exhibiting a yellowish hue suggesting an older stellar population. There is evidence of redder regions within the galaxy, potentially indicating areas of dust obscuration or the presence of older, redder stars. Overall, the galaxy appears relatively undisturbed, with no obvious signs of spiral arms or major tidal interactions, although a slight asymmetry suggests possible minor disturbances. It has an estimated size of roughly 2 kpc.
