The galaxy presents as a relatively smooth, elliptical structure. Its core exhibits a yellowish hue, suggestive of an older stellar population. The outer regions display a faint, diffuse glow with hints of reddish tones, potentially indicating some ongoing, albeit low, level of star formation or the presence of older red giant stars. The galaxy is not perfectly spherical, exhibiting a slight elongation in its shape. There is no evidence of a prominent disk or spiral arms, nor are there apparent signs of a major ongoing merger. The morphology suggests the galaxy is likely an early-type galaxy in a relatively quiescent state.
