The galaxy presents a somewhat elliptical morphology, appearing as a flattened disk oriented at an oblique angle to our line of sight. The central bulge exhibits a bright, concentrated luminosity, suggesting a high stellar density and/or the presence of an active galactic nucleus, though this is not definitively discernible from the image alone. The luminosity appears to decrease steadily toward the outer regions of the galaxy. The overall color profile shows a dominance of redder wavelengths, indicating an older stellar population and potentially lower ongoing star formation rates. There is some evidence of possible minor disturbances within the galaxy, and there are no apparent signs of ongoing major mergers or intense starburst activity.
