The galaxy presents a predominantly smooth morphology. The central region exhibits a bright, concentrated luminosity, suggesting a high stellar density. The overall shape appears somewhat elliptical, though not perfectly circular. There's a subtle elongation, with the galaxy appearing more "in between" round and elongated, rather than distinctly spherical or cigar-shaped. Evidence of a disk or distinct features is not immediately apparent. There appears to be no major merger or substantial tidal distortion, with only a slight, nearly imperceptible asymmetry. Color gradients suggest some variation in stellar populations or dust content within the galaxy, with the central region exhibiting a yellowish hue.