The galaxy presents as an elongated, cigar-shaped structure. A distinct color gradient is observable across the galaxy's body, with a relatively blue hue towards one end, transitioning to a warmer, yellow-orange hue towards the central region. This color variation may indicate varying stellar populations or dust distribution.

The galaxy appears to be undergoing significant interaction or disturbance, given its irregular morphology. There is a faint suggestion of tidal features, potentially hinting at an ongoing or recent merger event. The overall light distribution seems clumpy, and the galaxy lacks a clearly defined spiral arm structure or a prominent central bulge. It appears relatively small in extent, suggesting a dwarf galaxy. Based on its morphology, it would be classified somewhere between a irregular galaxy and a possible merger.
