The galaxy presents as a roughly elliptical object. The central region exhibits a high concentration of light, suggesting a prominent galactic nucleus or bulge. Moving outward from the core, a disk structure is visible. The structure appears to have some disturbances in the form of irregular light distribution. A hint of merging and tidal features or minor disturbances is suspected. Color gradients indicate a likely difference in stellar populations or dust content between the inner and outer regions. Specifically, the outer regions exhibit bluer hues compared to the slightly redder central region, potentially indicative of ongoing star formation in the disk.
