The galaxy presents a largely smooth and rounded morphology, suggestive of an elliptical or lenticular type. Its overall color appears relatively red, indicating a population of older stars and a potentially low rate of ongoing star formation. There is little evidence of spiral arms or significant dust lanes within the galaxy's structure. A slight elongation is noted, but there is no strong indication of a disk component. It is generally isolated, displaying no signs of major merger activity or significant tidal disturbances, although a minor disturbance cannot be entirely ruled out. Its moderate absolute magnitude suggests a galaxy of intermediate mass and luminosity within its redshift range. The galaxy's central region is the brightest, fading gradually towards the outskirts.
