The galaxy exhibits a distorted morphology, suggestive of an ongoing or recent interaction. A distinct, elongated arm appears to extend from the main galactic body, displaying a bluish hue indicative of potential star formation activity. A smaller, companion galaxy is situated relatively close to the primary galaxy, with some blurring between them. This lends further credence to the interaction hypothesis, and it is possible that the elongated arm is tidal debris. The central region of the main galaxy displays a relatively compact structure, although its overall form lacks well-defined spiral arms or a smooth elliptical profile. The light from the overall structure is faint, and the surface brightness of the galaxy appears relatively low. The edge-on nature of the main galaxy might be obscuring its detailed features.
