The galaxy appears as a moderately luminous, diffuse object, exhibiting a smooth and centrally concentrated morphology. The light profile suggests a relatively featureless structure, with no prominent spiral arms or distinct bar visible. The overall shape is approximately rounded, with a slight tendency towards an elliptical form. There are no signs of major merger activity or significant tidal disturbances, although a subtle irregularity in the outer regions can be observed. The color distribution within the galaxy is subtly varied, with a brighter and slightly bluer central region that fades gradually to redder hues in the outer parts. This color gradient may indicate ongoing, albeit relatively low, levels of star formation activity within the galactic core, contrasted by older stellar populations in the surrounding areas. Overall, this galaxy presents as a mature system undergoing slow and steady evolution.
