The galaxy presents a generally smooth morphology, with a centrally concentrated bulge. The overall shape appears elliptical or lenticular, showing a flattened disk-like structure oriented horizontally. The central region exhibits a bright, yellowish-white core, suggesting a concentration of older stellar populations. Moving outward from the core, a bluer hue becomes more prominent along the equatorial plane, possibly indicating regions of ongoing star formation. The galaxy's edges are diffuse, fading into the background sky, lacking sharp or distinct boundaries. There is no obvious evidence of spiral arm structures or significant tidal disturbances in this image. The relative smoothness of the light distribution points to a relatively evolved system dominated by older stars.
