The galaxy presents as a lenticular or possibly early-type spiral galaxy, viewed at a high inclination relative to our line of sight. It exhibits a moderate degree of central concentration, with a bright, yellowish core region that gradually fades into a more diffuse, outer disk. The disk appears relatively smooth and featureless, lacking prominent spiral arms or distinct dust lanes visible in the image. The overall shape is elongated, with an estimated physical radius of approximately 6.7 kpc. The color profile suggests an older stellar population, with a moderate amount of ongoing star formation. There are no obvious signs of recent major merger activity or significant tidal disturbances, although minor disturbances cannot be ruled out.
