The galaxy presents an overall elliptical morphology, appearing largely featureless. The light distribution exhibits a smooth profile, suggesting a relatively uniform stellar population. The central region displays a concentrated luminosity, potentially indicative of a galactic nucleus. A slight elongation is observed, deviating from a perfectly circular shape. Color gradients are subtle, with a hint of a redder hue towards the central bulge and a bluer tinge in the outer regions, which could point to variations in stellar age or metallicity. No distinct spiral arms or dust lanes are discernible, reinforcing the classification as an elliptical galaxy. There is no clear evidence of any major ongoing mergers or significant tidal disturbances.