The observed galaxy presents a primarily smooth morphology. There is little evidence of spiral arm structure or distinct features such as bars or rings. The galaxy exhibits an elliptical shape, appearing somewhat elongated. The light distribution is centrally concentrated, with a gradual decrease in brightness towards the outer regions. The core appears brighter, surrounded by a more diffuse halo. There's no prominent signs of tidal tails or distortions, suggesting no recent major merger activity. The color appears to be relatively uniform across the galaxy, with a hint of blue in the central core. This could indicate a population of younger stars in the core. The smoothness and color are consistent with an elliptical galaxy containing an older stellar population. The elongated shape could imply that the galaxy is not viewed face on, or that it may be a disk galaxy viewed at high inclination. There may be very minor disturbances in the outer regions, hinting at past interactions or minor mergers. 
