The galaxy presents as a centrally concentrated object, with a smooth, symmetrical morphology. It is largely featureless. The galaxy exhibits a color gradient, transitioning from a reddish core to a bluer halo. The lack of distinct spiral arms or other prominent features suggests a classification toward the elliptical end of the Hubble sequence. The smoothness and roundness of the light distribution is quite pronounced. There is no apparent evidence of ongoing major mergers or significant tidal disturbances affecting its structure, though a possible minor asymmetry can be seen on the bottom left of the galaxy. The central region shows evidence of recent or ongoing star formation, indicated by its reddish hue. The galaxy's blue halo suggests the presence of a population of younger, bluer stars, or a lower density of dust. Based on these characteristics, a preliminary classification as an early-type galaxy with a small amount of star formation could be considered.
