The galaxy appears as a relatively smooth, elliptical structure with a high degree of central concentration. The central region exhibits a yellowish-white hue, suggesting a population of older stars and minimal ongoing star formation. Moving outward from the center, the color shifts towards a slightly bluer tone, implying the presence of a younger stellar population or perhaps some residual star formation activity.

The galaxy's overall shape is generally ellipsoidal. There are hints of a slightly elongated structure, but no distinct spiral arms or bar features are visible. The galaxy appears relatively undisturbed, with no obvious signs of a recent major merger event. There may be a minor companion or tidal disturbance visible on one side.

The estimated size of the galaxy is relatively compact. The inferred mass places it within the range of typical spiral galaxies.
