The galaxy presents a relatively smooth, elliptical morphology. It appears elongated, exhibiting a cigar-like shape. There is little to no visible evidence of spiral arms or a distinct disk structure. The galaxy's light profile suggests it's dominated by an older stellar population, appearing relatively uniform in color and brightness across its body. There are no prominent signs of recent or ongoing major mergers. Faint disturbances may be present upon closer inspection, though the general structure of the galaxy appears largely undisturbed. 
