This galaxy exhibits an elliptical morphology, presenting a smooth, concentrated light distribution. The central region of the galaxy appears bright and yellow, suggesting an older stellar population is dominant here. Extending outward from the core, there is a transition to a bluer hue. This may indicate the presence of younger stars and ongoing, though perhaps subdued, star formation in the outer regions. The galaxy shows a slight flattening, with a departure from a perfect circular shape. There is no strong evidence of tidal disturbances or major mergers in the immediate vicinity, though subtle asymmetries in the outer regions indicate there could be minor gravitational interaction.
