The galaxy presents as a flattened, elongated system with a distinct central bulge. The light distribution suggests a relatively smooth morphology. The galactic disk appears oriented approximately edge-on from our line of sight, obscuring any apparent spiral arm structure. The central bulge exhibits a yellowish hue, possibly indicative of an older stellar population. The disk appears bluer than the central bulge, possibly due to the presence of younger, hotter stars and regions of ongoing star formation. There are no obvious signs of significant tidal disturbances, major mergers, or other morphological irregularities within the visible structure of the galaxy.
