The galaxy exhibits a flattened, disk-like morphology when viewed from our perspective. The light distribution appears smooth, with a relatively bright, concentrated central region which seems to be its bulge.  

There are subtle variations in color across the galaxy. The central bulge presents a yellower hue, indicative of a relatively older stellar population. Moving outward from the center along the major axis of the disk, the color gradually shifts towards bluer hues, this suggests the presence of younger, hotter stars. The bluer regions are not well-defined but instead diffuse. 

There does not appear to be clear evidence of prominent spiral arms, bars, or other strong morphological features within the disk. A small degree of morphological disturbance may be occurring within the disk, but no strong evidence of a recent or ongoing major merger is readily apparent. The overall symmetry and smoothness indicate the galaxy is relatively undisturbed.
