The galaxy appears to be an elliptical galaxy, likely a relatively massive system with a redshift of approximately 0.437. The object exhibits a smooth, centrally concentrated light profile with a fairly high degree of roundness. There is no clear evidence of spiral arms or a prominent disk. Faint hints of disturbances are visible in the outer regions, possibly indicative of a minor interaction or past merger event. The galaxy's color suggests it is primarily composed of older stellar populations, with relatively little ongoing star formation. The estimated size is relatively large, which, combined with the morphology, points to a well-evolved system.
