The galaxy presents as a smooth, elliptical-like structure, with a concentrated central bulge exhibiting a yellowish-orange hue. There is little to no visual evidence of spiral arms or distinct features within the galaxy. The overall shape is relatively rounded, transitioning smoothly from the bright core to a more diffuse outer halo. The color profile suggests an older stellar population, potentially with a relatively low rate of ongoing star formation. No signs of major mergers or significant tidal disturbances are apparent in the image. There may be a slight elongation but it is generally round, with no disturbances visible in the image.
