The galaxy presents as a somewhat distorted spiral galaxy, with one prominent, elongated arm. The core of the galaxy appears relatively smooth and centrally concentrated, with a yellow/white hue, indicative of an older stellar population. The spiral arm exhibits a bluer color, suggesting the presence of younger, hotter stars and ongoing star formation. There is a faint, diffuse glow surrounding the central bulge. The distortion in the spiral structure may suggest a possible past interaction with another galaxy or minor merger event. The overall structure is not perfectly symmetrical, which could also be indicative of internal dynamics or past interactions. The galaxy appears to have a low star formation rate with a relatively low mass. A notable feature is the extended arm, which seems to be tidal in nature.
