The galaxy presents as a moderately bright, flattened disk-like structure oriented nearly edge-on relative to our line of sight. A prominent dust lane bisects the galaxy horizontally, obscuring the central bulge and providing evidence of internal structure within the disk. The light distribution indicates a slightly brighter and more concentrated central region, suggesting the presence of a galactic nucleus or a dense stellar population at the core. The galaxy appears to have relatively smooth features overall, with no readily apparent spiral arms or significant irregularities. The morphology suggests a possible lenticular or early-type spiral galaxy, though the obscuration by the dust lane makes a precise classification difficult. Subtle color variations are observed across the galaxy's disk, potentially indicative of differences in stellar populations or dust content in different regions. There might be a very minor gravitational disturbance or tidal feature, but this is uncertain.
