The galaxy presents an elongated, cigar-shaped morphology. It appears relatively smooth in texture, lacking prominent spiral arms or distinct features within the disk. A central bulge is discernible, exhibiting a higher concentration of light. The galaxy displays a bluish hue, potentially indicating recent or ongoing star formation, though overall star formation is observed to be quite low. There is no evidence of a major merger event. Some minor disturbance or interaction is possible, but not easily discernible. Based on the observed ellipticity, the galaxy is viewed at a significant inclination.
