The galaxy presents an elliptical morphology, appearing as a smooth, somewhat diffuse object. It exhibits a concentrated central bulge that graduates outward into a less defined halo. Color gradients are subtle, with a yellowish core transitioning to a slightly bluer hue in the outer regions. This suggests a population of older stars concentrated centrally, with some ongoing star formation potentially occurring in the galactic outskirts. The overall shape is elongated, but not extremely so, indicating a moderate degree of ellipticity. There is no obvious evidence of spiral arms or prominent dust lanes, supporting the classification as an elliptical galaxy. The galaxy's light is relatively evenly distributed without any distinct features that would indicate recent merger events or significant tidal disturbances.
