The galaxy presents a largely smooth, elliptical morphology. Its core exhibits a high degree of central concentration, appearing bright and somewhat yellow-orange in color. The galaxy's shape is elongated, leaning toward a cigar-like profile, although the deviation from a perfect ellipse is moderate. No distinct spiral arm structures or prominent dust lanes are visible. There is little indication of ongoing or recent major merger activity, although the potential for minor disturbances in the galaxy's overall structure cannot be entirely ruled out. Faint, diffuse extensions of light are observed around the central bulge, which indicate an extended halo of stars and a gradual decrease in luminosity with increasing radial distance from the galactic nucleus. Overall, the galaxy exhibits properties consistent with an early-type galaxy, likely a lenticular or elliptical galaxy, based on its smooth appearance, and the concentration of its light distribution.
