The galaxy presents a morphology leaning towards smooth, though subtle features are discernible. It exhibits a flattened spheroid shape, closely approaching a disc. The central region is characterized by a concentrated, bright bulge, surrounded by a more diffuse and irregular disc-like structure.

Color gradients are present, with the central bulge displaying a yellowish to redder hue, suggesting an older stellar population. The outer regions of the disc show bluer tones, indicative of more recent star formation.

There's a suggestion of minor distortions or disturbances in the outer regions, though these are not pronounced enough to suggest a major ongoing merger. No obvious tidal tails or strong signs of recent major interactions are apparent.
