The galaxy appears as a slightly elongated, diffuse object. The central region exhibits a subtle concentration of light, suggesting a possible nucleus or bulge. The galaxy's color appears generally white to slightly yellowish, implying an older stellar population, although some faint blue hints could suggest recent star formation. There is no strong evidence of spiral arms. Overall, the galaxy appears relatively smooth in morphology. There is some visual suggestion of minor disturbances or tidal features, though this could be blending with background objects. These faint features, combined with the slightly irregular shape, indicate the possibility of an ongoing or past minor merger event.
