The galaxy presents a predominantly smooth morphology, suggesting a lack of significant spiral arm structures. The central bulge region exhibits a concentrated, bright yellowish hue, indicative of an older stellar population and potentially a supermassive black hole actively accreting material. Proceeding outwards, a less concentrated and bluer hue suggests a level of on-going star formation within the disk. Faint disturbances or minor asymmetric features are possibly present in the outer regions of the disk.
