The galaxy presents an elongated morphology, exhibiting a roughly cigar-shaped appearance. It is characterized by a central bulge, from which a diffuse disk-like structure extends. The color gradient suggests a higher concentration of older stellar populations within the central bulge, indicated by the relatively redder hue, and a bluer, possibly younger population within the disk. The overall smoothness suggests a system that has potentially undergone significant dynamical evolution, yet hints of disturbance are present in the irregular shape of the disk component, potentially indicating a past or ongoing interaction event. The galaxy's light profile appears to fade gradually from the core outwards.
