The galaxy presents as an edge-on or highly inclined spiral system. A prominent bulge is observed, centrally concentrated and exhibiting a smooth, featureless morphology. The disk component appears relatively thin and elongated, with visible dust lane absorption along the galactic plane, indicating significant obscuration. The light distribution across the galaxy appears centrally concentrated, with a gradual decrease in surface brightness moving outwards from the bulge towards the disk. The disk appears relatively symmetrical in shape, with no obvious signs of major tidal disturbances or ongoing mergers. There may be minor morphological disturbances, though not prominent. The dominant color is a yellowish white, which is indicative of an older stellar population and possibly low ongoing star formation rates.
