The galaxy presents a generally smooth morphology, suggestive of an elliptical or lenticular type. It has a somewhat elongated, cigar-like shape, with a visible color gradient. The central region appears brighter and bluer, indicating a higher concentration of younger stars or possibly an active galactic nucleus. Moving outwards from the core, the color appears to shift to a redder hue, indicating an older stellar population. No distinct spiral arms or prominent dust lanes are discernible. There is no major visual evidence of ongoing or recent merger activity, though some minor disturbance in the galaxy's halo cannot be ruled out. The overall appearance indicates a galaxy that is either relatively quiescent or has undergone significant morphological transformation.