The galaxy presents a distinctly elongated, cigar-shaped morphology. Its light profile appears smooth and centrally concentrated, with a gradual decline in surface brightness moving outward from the core. The core region exhibits a yellowish-white hue, possibly indicating an older stellar population dominating the central region. Fainter, blue-tinged light is visible at the extended edges suggesting the presence of younger stars. The overall structure appears undisturbed, showing no apparent signs of major mergers or tidal interactions. A possible minor disturbance is suspected along the northern edge of the galaxy.
