The galaxy presents as an elongated, cigar-shaped structure with a smooth, diffuse appearance. A brighter, more concentrated region is observed toward one end of the galaxy, suggesting a possible bulge or a region of enhanced stellar density. There is a fainter region opposite of the brighter end, appearing as an extension from the central body of the galaxy. There is no evidence of strong spiral arm structure or distinct dust lanes. Based on its general morphology, the galaxy is likely an elliptical, with some minor disturbance noted. Star formation rate appears low overall. The overall color of the galaxy is yellowish, which is indicative of an older stellar population.
