The galaxy presents as a thin, elongated structure viewed nearly edge-on. A bright, concentrated central bulge is evident, with a gradual decrease in luminosity extending outwards along the galactic plane. No spiral arm structures are discernible, possibly due to the edge-on orientation, or potentially the absence of well-defined spiral arms. The galaxy appears relatively smooth, with no prominent dust lanes or significant asymmetries that would immediately suggest a major ongoing merger event, though some minor disturbances cannot be ruled out. The color gradient shows a subtle shift, with the central bulge appearing slightly redder and the outer disk exhibiting a bluer hue, suggestive of a difference in stellar populations. The galaxy is estimated to be of moderate size and mass, with ongoing but low levels of star formation. The central bulge appears slightly boxy or rounded rather than exhibiting a sharp spherical shape. The overall structure suggests a late-type spiral galaxy, or possibly a lenticular galaxy.
