This galaxy exhibits a spiral morphology, with moderately wound arms extending from a central bulge. The bulge appears to have a moderate size relative to the disk. There appears to be a suggestion of a bar-like structure extending from the bulge through the disk. The spiral arms have a patchy, flocculent appearance, implying active star formation regions or dust lanes. There's a blue tinge throughout, indicating the presence of young, hot stars. The galaxy is tilted with respect to our line of sight, and the light appears slightly elongated rather than circular. There is no obvious sign of any major merging or other galactic disturbance.
