The observed galaxy presents a clear disk-like morphology seen almost perfectly edge-on from our vantage point. A prominent central bulge dominates the core region, appearing more luminous than the surrounding disk and exhibiting a yellowish-orange hue. This suggests a population of older stars within the bulge. The disk itself is relatively thin and extended, displaying a slight warp. The overall color of the galaxy appears relatively red, which could be caused by dust obscuration and potentially ongoing, but possibly slowing, star formation. There is some slight clumping or disturbance visible in the lower region, potentially indicating the presence of faint features or tidal interactions.
