The galaxy presents as a somewhat elliptical, yet largely amorphous object. The core is a bright, concentrated region, exhibiting a yellow hue. The outer regions show a noticeable decline in luminosity moving outward, with a less defined, smoother profile, and hints of bluer color. No clear spiral arm structures or distinct features are discernible. The morphology is suggestive of a galaxy in transition, with the light distribution and color gradients indicating a mix of stellar populations and star formation activity. It is difficult to assess whether the galaxy is undergoing any major disturbances or interactions based on this single image. The light output is relatively high, suggesting a system of significant mass and likely considerable star formation.
