The galaxy presents as a relatively elongated, disk-like structure. Its overall color gradient indicates a yellowish central bulge which transitions to a bluer disk. This suggests a mix of stellar populations, with older, redder stars concentrated towards the center and younger, bluer stars populating the outer disk. The galaxy displays a moderate level of dust extinction, particularly evident as patchy obscuration across the disk. The morphological characteristics suggest a spiral galaxy seen nearly edge-on, possibly an Scd type. Evidence of any strong spiral arm structure is not clearly visible from this angle, and the morphology suggests the presence of a relatively smooth stellar distribution across the disk. There is a slight distortion of the galaxy's shape indicating a potential tidal interaction event, although the disturbances are subtle. Overall, the galaxy seems to be in a relatively undisturbed state of evolution.
