The galaxy presents as an intermediate object, neither purely elliptical nor a well-defined spiral. It displays a central bulge that appears relatively smooth, with a higher concentration of light compared to the surrounding regions. This suggests an older stellar population. 

Extending from the central bulge is a fainter, disk-like structure. While spiral arms are not clearly resolved, there's a hint of asymmetry and some texture within the disk, suggesting the possibility of nascent or disrupted spiral features. The color is predominantly bluish-white, suggestive of at least some ongoing star formation within the disk.

There are also potential signs of interaction or past mergers, given the disturbed morphology. This could explain the subtle irregularities in the disk. The system appears to be in a relatively quiescent state of star formation.
