The galaxy presents a disk-like morphology, viewed at an angle neither face-on nor edge-on. There is a hint of spiral structure visible within the disk, with arm-like features extending from the central bulge. A central bulge is moderately prominent and concentrated. The disk appears somewhat asymmetrical and flocculent, with irregular patches of light. There might be evidence of tidal disturbances present, or some ongoing or past minor merger event. The overall color suggests a relatively quiescent galaxy with low star formation, dominated by an older stellar population. Some regions of bluer light are present, indicative of possible recent star formation. 
