The galaxy presents an elongated, cigar-shaped morphology. A pronounced central bulge, displaying a yellowish hue, dominates the core region. The surrounding disk exhibits a bluer color, suggestive of ongoing star formation. The disk appears relatively smooth, lacking prominent spiral arm structures. Faint dust lanes may be present within the disk, but the resolution prevents a definitive assessment. There is no visual evidence of a major ongoing merger, although subtle disturbances in the outer regions of the disk are not entirely ruled out. The galaxy's overall structure indicates a system undergoing a transition, possibly from a spiral to a more lenticular form.
