The galaxy presents as an elongated, cigar-shaped structure. The core region exhibits a concentrated, luminous glow. The overall color profile suggests an elliptical morphology with evidence of both older stellar populations in the central region and bluer star formation in the surrounding disk. The disk component shows some asymmetry, possibly indicating minor tidal interactions or internal disturbances. There is a small disturbance observed to the left of the core. The galaxy is relatively smooth in appearance.
