The galaxy presents a largely smooth and rounded morphology, with minimal discernible features such as spiral arms or a prominent disk structure. Its color profile is concentrated towards the redder end of the spectrum. This is most likely an elliptical galaxy. There is a concentrated central region which is slightly brighter than the rest of the galaxy. There is little to no evidence of ongoing mergers or significant tidal disturbances. The galaxy exhibits a generally uniform appearance across its body, suggesting a relatively homogenous stellar population.
