This galaxy presents as a disk galaxy, viewed at a slight angle, as it appears neither fully edge-on nor face-on. The central bulge is significant and exhibits a yellowish hue, suggestive of an older stellar population. A bluer tint becomes more prominent away from the bulge, indicative of younger, hotter stars and regions of active star formation in the disk. There are some signs of distortion and morphological features, such as slight asymmetry in the disk, which might imply that it is currently undergoing, or has undergone, some type of interaction or merger event. The overall light distribution appears relatively smooth.
