The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated, bright central region, suggestive of a significant galactic nucleus. The galaxy's color profile appears skewed toward the red end of the spectrum, with the core exhibiting a yellow hue. The surrounding halo gradually fades into the background, appearing slightly elongated vertically and exhibiting no distinct spiral arm features or significant dust lane obscuration. There are no obvious signs of major ongoing mergers or tidal disturbances. The observed morphology points towards a galaxy that is not actively forming many stars.
