The galaxy presents a generally smooth morphology, with the majority of light concentrated in a somewhat centrally located bulge.  There's a subtle, but noticeable disklike structure extending outwards from this brighter central region. The disk appears fairly uniform, with no clearly defined spiral arms or bar structure visible. 

Color gradients are present within the galaxy. The central bulge exhibits a yellowish-white hue, which may indicate an older stellar population. Progressing outwards towards the edge of the disk, there is a shift towards bluer tones. This bluer coloration likely signifies regions of ongoing star formation, although this activity is not pronounced based on the overall color distribution. The overall symmetrical shape suggests a system that hasn't experienced significant recent major mergers, although minor disturbances cannot be ruled out based on this image alone.
