The galaxy presents a complex morphology, appearing to be in a state of interaction or recent merger. The primary body of the galaxy displays an irregular shape with a relatively smooth texture, potentially indicating an elliptical or lenticular morphology that has been perturbed by a merging event. A distinct tidal tail or bridge-like feature is faintly visible extending from the main body, suggesting gravitational interaction with a smaller, possibly dwarf galaxy located nearby.

The color distribution within the galaxy is not uniform. The central region appears to be dominated by a yellowish-white hue, indicating the presence of an older stellar population. However, the overall color is not as red as it might be given the morphological type; there appear to be pockets of blue, suggesting regions of ongoing or recent star formation. The overall luminosity is considerable, hinting at a substantial stellar mass.
