The galaxy presents a somewhat smooth, elliptical morphology. It has a distinct, elongated shape, appearing cigar-like with an apparent lack of spiral arm structures. The central region exhibits a concentrated, bright yellowish-orange hue, potentially indicating an older stellar population. Moving outwards from the center, the color gradually fades into a fainter, diffuse bluish halo. There is no visual evidence of active galactic nuclei activity, such as a bright, unresolved core, nor is there any indication of tidal features or major disturbances indicative of recent major merger events. It is a relatively isolated galaxy, suggesting that it is not actively interacting with any other nearby galaxies. The galaxy is estimated to be at a redshift of approximately 0.21, placing it at a substantial cosmological distance. Based on its luminosity, its approximate size is around 9 kpc.