The galaxy appears as a smooth, elongated structure, suggestive of an elliptical morphology. The central region exhibits a yellowish hue, potentially indicating an older stellar population. Fainter, bluish light is observed in the outer regions of the galaxy, which could imply the presence of younger stars or ongoing star formation. The galaxy is significantly elongated, having a cigar shape appearance. There are no obvious signs of major mergers or tidal disturbances affecting the galaxy's structure.
