The galaxy presents a predominantly smooth morphology, suggesting an elliptical or lenticular classification. The light distribution appears concentrated towards the center, exhibiting a spheroidal structure. There is little evidence of spiral arms or significant dust lanes. Color gradients indicate a higher concentration of older stellar populations toward the galactic core, reddening the central region. The outer regions of the galaxy show a bluer hue, potentially indicating the presence of younger stars or a small amount of ongoing star formation, albeit at a low rate. There may be a small companion galaxy to the south of the primary galaxy. No significant signs of major merging activity are apparent in the image, however some minor disturbance cannot be ruled out.
