The galaxy presents as a slightly tilted, disk-shaped structure. A central bulge is discernible, appearing somewhat bright and concentrated, possibly indicating a dense population of older stars. The surrounding disk appears relatively smooth with a faint greenish hue, indicating a low amount of ongoing star formation. There is no indication of strong spiral arms or a bar structure. The galaxy appears relatively isolated, showing no significant signs of tidal disturbance or interaction with other galaxies. The overall color suggests a mix of stellar populations, with an older population dominating, and a small amount of younger stars.
