The observed galaxy presents as an elongated, cigar-shaped structure, suggesting an elliptical morphology. A central bulge region appears with a yellowish hue, potentially indicating an older stellar population. The outer regions display a bluer tint, suggestive of ongoing star formation, though the smooth appearance may indicate that the rate of star formation may be low. There is no prominent disk-like structure or spiral arm morphology visible. The galaxy appears relatively undisturbed, showing no strong signs of tidal interactions or recent major mergers.
