The galaxy presents as a somewhat elongated structure. Its central region appears relatively smooth and homogenous in color. Extending from the central region are fainter extensions, perhaps indicative of a disk-like morphology viewed at a steep angle. These extensions appear more disturbed and uneven in brightness, possibly due to dust lanes or active star formation regions. Overall, the galaxy exhibits a relatively blue color, suggesting the presence of a population of younger, hotter stars. There is no obvious evidence of a major ongoing merger, but the galaxy does appear slightly disturbed, which could suggest a past or minor merger event. The light distribution suggests a galaxy with an intermediate mass and a moderate star formation rate.
