The galaxy presents a generally smooth and elliptical morphology. It has a dominant central bulge with a relatively high degree of roundness. There's minimal evidence of spiral arm structure or significant disk features. The galaxy's color profile suggests a relatively evolved stellar population with a redder overall hue, transitioning towards bluer color as the radius increases. There may be minor disturbances in the galaxy's structure, but no major merging events are apparent. The overall luminosity indicates a reasonably massive galaxy.
