The galaxy presents as a smooth, elongated structure. Its morphology suggests an elliptical type, likely a spheroid system based on its cigar-like shape. The color profile indicates a relatively low star formation rate with a redder overall appearance, showing older stellar populations dominating the light emission. The central region displays a concentrated, bright core, possibly indicative of an active galactic nucleus or a dense stellar cluster. The lack of apparent spiral arms or distinct dust lanes further supports its classification as an elliptical galaxy with minimal ongoing star formation. The galaxy does not exhibit any signs of major disturbances or merging events based on its symmetric structure.
