This galaxy presents a generally smooth morphology. The central region appears to be a bright, concentrated bulge with a yellowish-white hue, suggesting an older stellar population. Surrounding this bulge is a more diffuse, bluish disk component. There is no clear spiral structure or defined arms visible. Some faint features or minor disturbances might exist in the outer regions, but the overall impression is of a galaxy with a predominantly smooth structure, possibly an elliptical or lenticular galaxy with ongoing, but relatively low, star formation. The blue color suggests the presence of some younger stars. There is no evidence of a major merger or strong tidal interactions with other galaxies.
