The galaxy presents a smooth, elongated morphology, exhibiting a distinct cigar-like shape. The central region displays a concentrated luminosity, appearing yellowish-white, which may indicate an older stellar population. Fainter, blue-tinged regions extend outward from the central bulge, potentially indicating areas of more recent star formation. The overall structure suggests minimal disruption, without any clear signs of major merger activity. A small area on one side of the galaxy is slightly extended, though without obvious signs of interaction, suggesting a possible minor disturbance. The galaxy exhibits a moderate level of star formation, though not a particularly high one.
