The galaxy presents as a somewhat elongated structure with a moderate degree of internal organization. The morphology appears intermediate, showing characteristics of both smooth and disk-like systems, though there is a lack of clear spiral arm definition. The central region exhibits a concentrated luminosity, potentially indicating a bulge component. The light distribution suggests it may be transitioning from a more featureless elliptical to a spiral.

The overall color index is moderate, transitioning from blue-green to red-orange as you move towards the core, indicating potentially older stellar populations present. However, the presence of a bluer hue in some regions indicates ongoing or recent star formation, particularly in the outskirts. There isn't any noticeable dust lane, and the overall structure appears relatively undisturbed, showing a lack of any major distortions or tidal features indicating a merger. Some degree of minor disturbance cannot be ruled out.
