The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high surface brightness with a yellowish hue, suggestive of an older stellar population. Moving outward, the galaxy displays a gradual decrease in surface brightness, with a faint, diffuse halo. There's minimal evidence of spiral arms or distinct features typically associated with disk galaxies. Slight disturbances or minor irregularities in the outer regions hint at potential past interactions, but the overall morphology appears generally undisturbed. The galaxy's shape is moderately elliptical, trending towards round rather than elongated or cigar-shaped. There is a hint of blue at the very edges of the halo, possibly indicating a small amount of recent star formation.
