The galaxy appears as a relatively compact object with a smooth, elliptical morphology. The core exhibits a concentrated luminosity profile, suggesting a high density of stars towards the center. A slight color gradient is discernible, transitioning from a more yellowish hue in the core to a marginally bluer tone in the outer regions. This subtle shift in color potentially signifies a change in stellar populations, with older, redder stars concentrated in the center and a younger, bluer population possibly extending further out. There are no discernible spiral arms or other distinct features.
