The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The core exhibits a bright, yellowish hue, suggesting a population of older stars. The isophotes are generally elliptical, showing a slight deviation from perfect circularity. There is a subtle color gradient moving outwards from the core, transitioning to slightly bluer hues in the outer regions, indicative of some ongoing star formation. No prominent spiral arm structures or dust lanes are discernible. There are no signs of active galactic nuclei or tidal disturbances.
