The galaxy presents a generally smooth, elliptical morphology. It exhibits a high degree of central concentration, with a bright, moderately defined core. The isophotes are elongated, appearing cigar-shaped, suggesting some degree of ellipticity. The galaxy is yellowish, possibly indicating an older stellar population with relatively little ongoing star formation. There is little evidence of spiral arm structure or dust lanes. A slight asymmetry is noticeable within the outer regions of the galaxy, potentially suggesting a minor interaction or disturbance, although no clear signs of mergers or major disturbances are immediately apparent.