The galaxy presents as an elliptical morphology, with a smooth and centrally concentrated light profile. The core region is dominated by a yellow-white hue, suggesting a population of older stars. Moving outwards from the center, the colour gradually shifts towards redder tones in the disk, indicating possible ongoing or recent star formation in the outer regions. Some very faint arms may be visible close to the bulge. The galaxy displays a round shape, though a slight elongation can be noticed. No obvious major disturbances or signs of interaction with other galaxies are readily apparent.