The galaxy presents as a somewhat elongated object, though its morphology appears relatively smooth. There is evidence of some asymmetry, particularly in the distribution of light. The central region exhibits a higher concentration of luminosity, suggestive of a galactic bulge or core. The color profile suggests a relatively evolved stellar population, with a dominant reddish-orange hue. The outer regions appear less defined, possibly indicating a more diffuse distribution of stars or gas in the galactic disk. There are indications of minor disturbances or interactions, observable as slight distortions in the overall shape. However, there is no clear sign of on-going mergers.
