The galaxy presents as a somewhat asymmetrical spiral type, viewed at an oblique angle relative to the observer. A substantial central bulge dominates the galaxy's luminosity, exhibiting a moderate concentration. Faint spiral arm structures are visible extending outwards from the central bulge.

There is a slight indication of a bar feature present in the galaxy's core, though it doesn't appear to be particularly strong. The galaxy does not appear to be an edge-on disk galaxy; it shows a degree of resolved structure.

A portion of the disk appears smoother than the spiral arms, suggesting a more uniform distribution of stars. This suggests it may be more of a transition galaxy that is in between an elliptical galaxy and a spiral galaxy.

There is a suggestion of a potential tidal interaction or minor disturbance, based on slight distortions in the outer regions. The presence of these asymmetries could indicate a past merger event. However, the galaxy does not present strong evidence of an ongoing or recent major merger.
