The galaxy presents as a generally smooth object, with a slight elongation along its major axis. It appears to be largely devoid of significant spiral arm structures or prominent dust lanes. The central bulge region exhibits a higher surface brightness, characterized by a yellow-white hue, suggesting an older stellar population. The outer regions of the galaxy show a gradual decrease in surface brightness and a slight shift towards bluer colors, potentially indicating the presence of younger, hotter stars. The overall morphology suggests a possible lenticular or early-type spiral galaxy, with a relatively high degree of symmetry. There is no obvious evidence of active galactic nuclei or recent major merger events, although some minor tidal disturbances cannot be entirely ruled out based on this image alone.
