The galaxy presents a morphology suggestive of a disrupted spiral or perhaps a galaxy undergoing a significant interaction. The main body of the galaxy is moderately smooth, appearing somewhat elliptical, and exhibits a yellowish-white color profile, possibly indicating an older stellar population within the central bulge. Emanating from one side of this main body is a pronounced, elongated tidal tail that curves away from the primary structure. This tail displays a gradient in color, shifting from a yellowish hue near the galaxy's center to a bluer tint further along its extension, hinting at the presence of younger stars in the outer regions of the tail. The overall shape is elongated, slightly cigar-shaped. There is evidence of some disturbances within the galaxy's structure, pointing towards possible past or ongoing gravitational interactions with another galaxy or a recent merger event. The galaxy is relatively compact, suggesting that it is a smaller galaxy.
