The galaxy appears to be a relatively face-on spiral or lenticular galaxy, with a bright central bulge. The bulge exhibits a yellowish-white hue, suggestive of an older stellar population. Surrounding the bulge is a fainter, bluish disk. While not clearly resolved, hints of spiral arm structure are present, though somewhat indistinct and patchy. The blue color suggests ongoing star formation within the disk. The galaxy appears somewhat smooth in overall texture, indicating a relatively low rate of current star formation activity. There is no obvious evidence of a major ongoing merger, although some minor disturbances or tidal features might be present upon closer inspection. The overall morphology suggests a transition from a more actively star-forming spiral towards a more quiescent, bulge-dominated system.
