The galaxy presents as a luminous elliptical, exhibiting a smooth, concentrated morphology. The light distribution appears centrally peaked, with a gradual decrease in surface brightness towards the outer regions. Its shape is moderately elongated, not perfectly spherical. There is no apparent spiral structure or distinct disk component. The color profile suggests an older stellar population, with a redder hue dominating the galaxy's overall appearance. No major signs of recent merger activity or strong tidal disturbances are observed, though there may be some minor asymmetries. The estimated size indicates that it is a relatively small galaxy.
