The galaxy presents as a somewhat diffuse, elongated structure. Its overall color appears to be bluish-white, suggesting a population of relatively young, hot stars. The light distribution suggests a dominant bulge component. The galaxy exhibits a flattened, disk-like morphology. The dust lanes are not distinctly observed. The ellipticity is quite high, indicating a highly inclined viewing angle. No prominent spiral arms or bar structures are discernible in this image. There is little sign of ongoing merging or tidal disruption. The overall impression is that of a relatively undisturbed galaxy with a smooth light profile.
