The galaxy presents a generally smooth, yet somewhat disturbed morphology. It is neither perfectly elliptical nor a clear spiral, exhibiting a shape that is somewhere in between, with an apparent elongation. There appears to be a brighter, more concentrated central region which could indicate the presence of a galactic nucleus or a bulge. The color profile appears to be predominantly bluish, suggesting a significant population of younger, hotter stars and ongoing star formation activity. Faint, diffuse extensions or tidal features are tentatively visible, hinting at possible past or ongoing interactions with another galaxy or a minor disturbance event. The galaxy does not appear to be undergoing a major merger, although some level of disturbance can be noted. The overall color and shape suggest an intermediate type galaxy, possibly a lenticular galaxy undergoing some sort of interaction.
