The galaxy presents a moderately elliptical morphology, with a significant central bulge. The color profile suggests a dominant population of older stars, exhibiting a yellowish-red hue, especially concentrated towards the galactic center. Faint indications of a disk component are present but not sharply defined. There is a slight asymmetry with minor disturbances and no clear signs of spiral arm structure or significant dust lanes visible in the image. The central bulge appears quite prominent and smooth, transitioning outward into a more diffuse and less concentrated halo. There's no sign of a clear tidal tail. The color indices indicate significant levels of redder light. Given the smoothness, color, and central concentration, this could be an early-type spiral or an elliptical galaxy.