The galaxy presents as a generally smooth, ellipsoidal structure. The core exhibits a concentrated, yellowish-orange hue, suggesting an older stellar population and minimal recent star formation in the galactic nucleus. A faint, diffuse greenish halo surrounds the central bulge, extending further along the major axis of the ellipse than perpendicular to it. This halo may indicate ongoing, albeit low-level, star formation in the outer regions of the galaxy, or it could be the remnants of a tidal interaction, although no obvious signs of a major merger or significant disturbance are visible. The galaxy's overall shape is intermediate between round and elongated, leaning more towards an elliptical morphology, with a slight cigar-shaped appearance. There are no clear signs of spiral arms or a distinct disk structure.
