The galaxy presents as an edge-on spiral system. A distinct, elongated central bulge is visible, exhibiting a smoothly distributed luminosity gradient. The bulge appears to be rounded. The disk component is significantly flattened, extending along the major axis. Internal structure within the disk is not readily apparent; it is generally featureless. There is no evidence of a prominent dust lane. The overall color is consistent with an evolved stellar population, with the central bulge appearing yellower than the disk. We do not observe any major tidal disturbances or signs of an ongoing merger event. There is no substantial presence of recent star formation.
