The galaxy appears as a centrally concentrated, yellowish object with an elliptical morphology. It exhibits a relatively smooth, featureless structure, lacking any apparent spiral arms or significant dust lanes. The light distribution suggests a higher concentration of older stellar populations within the central region, as evidenced by the yellow-red hue, which gradually fades into a more indistinct, diffuse outer region with a hint of bluer tones, suggestive of some younger star formation, although at a low rate. Overall, the galaxy's morphology leans toward a relatively undisturbed system with no clear signs of major mergers or tidal disruptions. The galaxy presents an intermediate ellipticity, neither perfectly round nor highly elongated.
