The galaxy appears to be a spiral, viewed at an oblique angle, with its disk tilted relative to our line of sight. The central bulge is prominent and appears relatively bright, suggesting a significant population of older stars. Faint spiral arms are observed extending from the central region, but their structure is somewhat irregular and ill-defined. The bluer tint observed in the arms suggest ongoing star formation is active here. There is a hint of a bar-like structure extending through the central region, though it is not particularly pronounced. The galaxy exhibits a moderate ellipticity, and appears somewhat flattened.
