The galaxy presents as a lenticular or edge-on spiral type, displaying a notable elongation. It possesses a relatively smooth texture, with a concentrated central bulge that appears yellow-orange in color, suggesting an older stellar population. The main body of the galaxy exhibits a flattened disk-like structure, oriented at a high inclination relative to our line of sight. A faint, diffuse halo may be present, though it blends with the background noise. The galaxy does not show signs of major recent mergers or significant tidal disturbances, although there may be hints of minor irregularities in its outer regions. There isn't prominent dust lane obscuration visible in the central regions. The color gradient suggests decreasing star formation rates.