The galaxy appears to be a relatively luminous, early-type system, possibly an elliptical or lenticular galaxy. It exhibits a smooth, centrally concentrated light profile with a high degree of rotational symmetry. The shape is elongated, appearing somewhat cigar-shaped. There is no obvious presence of spiral arms or significant dust lanes. The color is consistent with an older stellar population, exhibiting a redder hue. There is no strong evidence of recent star formation or ongoing merging activity, although a minor disturbance cannot be ruled out. Overall, the galaxy seems to be a well-established system with a significant stellar mass and a relatively low star formation rate.
