The galaxy presents as a somewhat elongated structure, with a brighter, more concentrated central region likely corresponding to the galactic bulge. The galaxy appears tilted relative to our line of sight, possibly an edge-on or highly inclined spiral. There's a subtle color gradient across the galaxy, with the central bulge exhibiting a yellower hue, potentially indicative of an older stellar population and less active star formation. The outer regions appear slightly bluer, which may be related to the presence of younger, hotter stars. Overall, the galaxy lacks any obvious signs of major disturbance or recent merger activity. Faint hints of disk-like structures are potentially visible. The galaxy's apparent smooth texture suggests a relatively evolved system.
