The galaxy presents a moderately bright central bulge, exhibiting a yellowish-orange hue, suggestive of an older stellar population. Surrounding the bulge, a more diffuse, bluish disk is observed. The disk appears relatively smooth, with only subtle indications of spiral arm structure. The bluer color of the disk implies the presence of younger, hotter stars and ongoing star formation. There are possible disturbances. The overall morphology indicates a galaxy with characteristics intermediate between a spiral and an elliptical galaxy, potentially an early-type spiral or a lenticular galaxy undergoing some star formation.
