The galaxy presents a somewhat elongated, cigar-shaped morphology. It appears to be a relatively smooth object, lacking prominent spiral arms or significant irregular features. The central bulge exhibits a yellowish hue, suggesting an older stellar population. Moving outwards from the core, the disk appears fainter and slightly bluer, potentially indicating ongoing star formation. There is no obvious evidence of any major mergers or strong tidal disturbances, although a minor asymmetry cannot be ruled out. The overall structure suggests a galaxy transitioning towards a lenticular or early-type spiral morphology, with a dominant bulge and a subdued disk.
