The galaxy presents with a generally indistinct morphology, exhibiting a moderately diffuse structure. A prominent, albeit subtle, central bulge region is suggested by a slight increase in luminosity towards the center. The overall color profile indicates a population of intermediate-age stars with some regions of bluer light, possibly indicating ongoing star formation. There is a lack of well-defined spiral arms, but some patchiness is present, which suggests a more disturbed morphology, perhaps due to gravitational interactions or recent merger activity. The features are subtle and a significant portion of the galaxy seems to be amorphous in nature. Faint tidal features or minor disturbances may be present, suggesting that the galaxy is undergoing a merging event. These disturbances contribute to the irregular structure and indicate that it has a complex and dynamic system. 
