The galaxy presents as a somewhat elongated, disk-like structure. It is observed nearly edge-on. There is a central bulge region which appears to be the brightest, densest part of the galaxy. This central region exhibits a smooth, concentrated light distribution, suggesting a population of older stars. The disk itself is less luminous, with a subtle blue hue indicating the presence of younger, hotter stars and possibly ongoing star formation. The disk extends outwards from the central bulge. There is little evidence of spiral arm structure or significant dust lanes in this particular view, with slight asymmetry on each side of the central bulge. There do not seem to be any signs of a major merger, but minor interactions cannot be ruled out given the irregularity within the structure.
