The galaxy presents a predominantly smooth morphology, exhibiting a diffuse, elliptical shape. The color profile suggests a higher concentration of older stellar populations, leaning toward redder hues. There is a slight asymmetry to the galaxy’s overall light distribution; there may be a minor disturbance. The central region appears brighter than the outer regions, potentially indicating a higher density of stars or a more active galactic nucleus, though the resolution is not sufficient to confirm this. The image quality limits detailed analysis of internal structures, such as spiral arms or dust lanes.
