The observed galaxy presents as a late-type spiral galaxy, likely viewed edge-on. A prominent central bulge is visible, exhibiting a concentrated luminosity. The galaxy demonstrates an elongated morphology with a high degree of axial symmetry. The disk appears thin. The apparent major axis of the disk spans a small angle. There are no obvious signs of ongoing major mergers or significant tidal disturbances. The galaxy exhibits a relatively smooth light distribution across its disk, with no discernible distinct spiral arm structures. The bulge appears to be centrally concentrated and primarily spheroid in shape. The galaxy's colors suggest a moderate stellar population with some ongoing star formation.
