The galaxy presents as an elongated, somewhat cigar-shaped structure. It exhibits a smooth overall appearance, with a central bulge that is distinctly brighter and displays a reddish hue. Moving outward from the central region, a more diffuse disk-like component can be observed, characterized by a bluer color profile, potentially indicative of ongoing star formation. There are no obvious signs of major disturbances or a recent merger, although subtle asymmetries might suggest minor interactions. The light distribution is relatively concentrated, with a significant fraction of the luminosity emanating from the central region.
