The galaxy presents an elongated, cigar-shaped morphology. It exhibits a relatively smooth and featureless appearance in the optical bands. The central region appears brighter, suggesting a concentration of stars and possibly an older stellar population dominating the core. A faint, diffuse halo surrounds the central bulge, extending along the major axis of the galaxy. Subtle color gradients are visible, with a slightly bluer hue in the outer regions, possibly indicating ongoing, albeit low, levels of star formation compared to the redder, presumably older, stellar populations in the central region. There are no apparent signs of significant disturbances or major merger activity. The galaxy appears largely undisturbed, representing a relatively evolved system.
