The galaxy presents as a centrally concentrated, likely elliptical, system. Its overall shape is elongated, exhibiting a cigar-like morphology. The central region displays a distinct yellowish-white hue, suggesting an older stellar population dominating the core. Fainter bluish extensions are visible along the major axis, possibly indicative of some ongoing star formation. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions, though minor disturbances cannot be ruled out.
