The galaxy presents as an elongated, cigar-shaped structure, suggesting a possible elliptical morphology. The central region is brighter and more condensed, indicative of a higher stellar density or an active galactic nucleus. There appears to be a subtle color gradient along the major axis, transitioning from a bluish hue at one end to a reddish hue at the opposite end. This color variation may indicate differing stellar populations or dust content along the galactic body. There seems to be some low level of disturbance or asymmetries possibly indicative of an ongoing or recent minor merger event. No distinct spiral arms are readily discernible. Overall, the galaxy exhibits characteristics of a galaxy undergoing some kind of evolutionary process.
