The galaxy presents as an edge-on spiral system. The dominant feature is a prominent, moderately bright central bulge which appears to have a smooth and somewhat rounded morphology. The disk is thin and elongated, with the majority of its light concentrated towards the central bulge. There is a suggestion of dust lane obscuration along the mid-plane of the disk, although the image resolution limits detailed analysis. Overall, the galaxy exhibits characteristics consistent with a relatively massive system, with evidence of ongoing but perhaps not intense star formation. There are no readily apparent signs of major mergers or significant tidal disturbances, but some minor disturbances in the disk cannot be ruled out. The disk shows some bluer light but appears redder than the bulge, suggesting a population of older stars.
