The galaxy presents as a moderately luminous object with a distinct elongated morphology, approximating a cigar shape. A substantial fraction of the light appears to be emitted from a smoother component, possibly a bulge or halo, while the presence of a fainter disk-like structure is suggested by the slightly flattened form. It is primarily yellowish-orange in color, indicating an older stellar population and lower levels of ongoing star formation. There may be some minor disturbances in the morphology, but the primary structure appears relatively undisturbed with no signs of significant mergers.
