The galaxy presents as a slightly elongated, yet largely rounded, structure. Its overall color appears to be a warm yellowish hue, suggesting an older stellar population with fewer hot, young stars contributing to the bluer wavelengths. A brighter, more concentrated central bulge is observed. Fainter, seemingly disturbed arms or extensions are seen to emanate from the central region, hinting at potential past interactions or mergers. These faint features exhibit a slightly bluer coloration relative to the central bulge, potentially indicating regions of ongoing or recent star formation. Overall, the galaxy exhibits characteristics of a system experiencing a mix of quiescent evolution and minor disturbances.
