The galaxy appears to be of intermediate size. It has a somewhat diffuse morphology, lacking a clear, well-defined structure. There is a suggestion of a central bulge-like concentration, but it's not strongly pronounced. The galaxy exhibits a faint, hazy appearance, with no distinct spiral arms or bar structures readily visible. The overall color is somewhat blue-green, which could indicate ongoing star formation, although the faintness of the object makes precise color determination challenging. The light distribution is not entirely smooth, suggesting some degree of irregularity or possible interaction. There is potentially evidence of minor tidal disturbances or merging activity in the form of slightly extended, diffuse features. The possibility of artifacts affecting the perceived morphology must be considered given the galaxy's faintness. Further investigation with higher resolution imaging and spectroscopic analysis would be needed to better constrain the galaxy's morphology, star formation rate, and evolutionary state.
