The galaxy presents as a spiral type, observed at a slight angle relative to our line of sight. A central bulge is apparent, exhibiting a bright, concentrated luminosity, indicative of a significant stellar population. The spiral arms are well-defined, extending outwards from the bulge. The winding of the spiral arms appears relatively tight. There appears to be at least two spiral arms. The galaxy exhibits a disk-like morphology. A degree of internal structure is visible within the arms, suggesting regions of ongoing star formation. The light distribution in the disk appears uneven, implying varying densities of stars and interstellar matter. There appears to be a weak bar feature extending through the central region of the galaxy. There is no immediately obvious evidence of a major merging event or strong tidal disturbances.
