The galaxy exhibits a somewhat elongated, cigar-like morphology. The central region presents a smoother appearance with a slightly concentrated bulge suggesting an older stellar population. Moving outwards from the center, there is a faint disk. There is a possible indication of some form of disturbance in the disk. The overall blueish tint indicates the presence of some ongoing star formation, although it appears to be relatively low. The galaxy does not appear to be undergoing a major merging event, but there are hints of a minor interaction.
