The galaxy presents as a smooth, elongated structure, suggesting a likely classification as an elliptical galaxy. The morphology appears cigar-shaped, with a distinct axis of elongation. There is little evidence of spiral arms or a prominent disk. The color is relatively uniform across the galaxy, tending towards a redder hue, which implies an older stellar population with reduced ongoing star formation. The overall smooth appearance indicates that it is a well-formed galaxy with a degree of morphological maturity. There is no obvious dust lane obscuring its form, and no indication of tidal interactions or mergers. The galaxy does not appear to be undergoing any significant disturbances or active galactic nucleus activity based on its appearance.
