The galaxy presents as a relatively faint, elongated object. Its morphology is primarily disc-like, with the longest axis stretching roughly five times its shortest. The central region exhibits a subtle bulge, appearing smoother and more concentrated. The color gradient suggests a mix of stellar populations; the core has a yellowish hue, transitioning to a bluish tint toward the outer regions. The bluish color in the outer disc potentially indicates ongoing or recent star formation activity. There is no indication of active galactic nuclei, tidal tails or major disturbances from merging. The shape of the galaxy is primarily cigar shaped.
