The galaxy appears as a slightly elongated, disk-like structure viewed at an oblique angle. The central region exhibits a concentrated, bright core, suggesting a significant population of older stars or a possible active galactic nucleus, though further spectroscopic data would be needed to confirm the latter. The galaxy's light appears to be dominated by redder wavelengths in the central bulge. The outer regions of the galaxy show a less defined structure, with a bluer tint that may indicate the presence of younger stars, possibly in the spiral arms of the galaxy. The overall morphology does not show signs of major tidal disturbances or ongoing merger events. There are only faint disturbances within the galaxy. The galaxy is relatively smooth in appearance.
