The galaxy presents as a largely smooth, elliptical-like structure with a concentrated central bulge. Its light profile appears relatively uniform and lacks prominent spiral arm features. A slight elongation is observed but not distinctly cigar shaped, suggesting a somewhat rounded morphology. The light emitted from the galaxy is primarily in the redder wavelengths, indicating an older stellar population dominating the light output. There may be some hints of a very faint disk-like structure, but no dust lanes are visible. No signs of active galactic nuclei (AGN) features such as jets or a strong point source are present. There is a potential companion galaxy which shows a redder hue to it, suggesting it is an older galaxy. There are no signs of any active merging events or major distortions in the galaxy's shape and it appears to be undisturbed.
