The galaxy presents as a single, relatively smooth object. The morphology is elliptical in nature, appearing largely spheroidal with no prominent spiral arm structures or a distinct disk component visible. A central concentration of light is apparent, suggesting a bulge or active galactic nucleus, possibly obscured by dust. The color profile indicates a yellow-red hue, which is characteristic of older stellar populations, lower rates of star formation, and potentially dust extinction. There is little evidence of ongoing mergers or major disturbances in the galaxy's structure. The galaxy has an apparent small angular size in the image, which may indicate significant distance. 
