The galaxy appears to be a luminous elliptical galaxy, exhibiting a smooth, featureless morphology. It possesses a high degree of central concentration, with the majority of the light emanating from the core. The galaxy presents a slightly elongated shape, falling somewhere between round and cigar-shaped. There is no obvious indication of spiral arms or other disk-like features. The colour profile indicates the dominance of older stellar populations, suggesting a low star-formation rate. There is no evidence of ongoing major or minor mergers, however, there could be some minor signs of disturbance. Based on the estimated size and brightness, this galaxy appears to be a massive system.
