The galaxy presents a largely smooth morphology with a concentrated central bulge. The light profile transitions smoothly from a bright, yellowish core to a fainter, bluer outer region. There is little indication of spiral arms or significant dust lanes. The overall shape is nearly circular, exhibiting a high degree of radial symmetry. The galaxy displays a color gradient, with the core appearing relatively redder than the outer regions, which exhibit a bluer hue. There is no visual evidence of strong tidal disturbances, major mergers, or ongoing interactions with other galaxies, suggesting a relatively undisturbed system. The galaxy's light is distributed over a moderate angular size.