The galaxy appears to be an elliptical type, characterized by a smooth, spheroidal morphology. The light distribution is centrally concentrated with a gradual decrease in surface brightness towards the outer regions. There is no evidence of spiral arms or a prominent disk. The galaxy appears elongated, with a cigar-like shape. The color suggests a population of older stars. It shows no signs of active star formation. There is no visible evidence of any major ongoing merger activity or significant tidal disturbances.
