This galaxy presents as an edge-on spiral, exhibiting a flattened disk-like structure oriented nearly perpendicular to our line of sight. A prominent central bulge is visible, appearing smooth and concentrated, with an orange hue. The disk itself appears relatively smooth, with minimal indication of distinct spiral arm structures or prominent dust lanes. The overall color profile suggests a population of older stars. The disk's edge appears relatively well-defined. No signs of ongoing major mergers or tidal disturbances are apparent from visual inspection of the galaxy's morphology.
