The galaxy presents as a relatively smooth, intermediate system with some distinct features that suggest ongoing or recent interaction.

The galaxy exhibits a somewhat round morphology, but deviations suggest disturbances. There is evidence of asymmetry in the galactic structure, with possible tidal tails or distortions extending from the main body. These features suggest gravitational interaction, possibly a minor merger or tidal disruption. Color variations within the galaxy could indicate regions of varying stellar populations or dust obscuration. 

In certain regions, there appears to be evidence of star formation or regions of enhanced luminosity. The galaxy does not appear to be a pure elliptical, spiral, or irregular type but rather a transitional object potentially undergoing morphological transformation due to internal or external processes.
