The galaxy appears to be a spiral type, observed at an oblique angle to our line of sight. The central bulge is prominent and displays a yellowish hue, indicative of an older stellar population. Faint spiral arms are visible extending outwards from the central bulge. These arms are not tightly wound, suggesting a later-type spiral classification. There appears to be a moderate amount of ongoing star formation, as hinted by the bluer color observed in the arms. The galaxy does not exhibit any obvious signs of a major merger, though subtle disturbances might be present upon closer inspection.
