The galaxy presents as a diffuse object with a roughly elliptical morphology. The core appears relatively smooth and centrally concentrated, with a gradual decrease in luminosity extending outwards. There is some suggestion of substructure within the galaxy's halo, but image resolution limitations hinder a definitive assessment. The color profile appears relatively uniform across the galaxy, with only subtle variations. Overall, the galaxy presents a morphology consistent with an elliptical type system, exhibiting minimal signs of spiral arms or significant star formation regions. There is no apparent distortion or tidal features, which suggests that there have been no major mergers, or significant gravitational interactions in the recent past. 
