The galaxy presents a relatively smooth morphology. Its structure appears to be dominated by a central bulge or spheroid component. This bulge exhibits a yellowish hue, which suggests a population of older stars, potentially with lower ongoing star formation activity.

A distinct, bluish feature is observed closer to the bottom, indicating a possible region of active star formation. This blue region might correspond to a spiral arm segment or a clump of younger, hotter stars within the galaxy.

Evidence of merging or tidal disturbances appear present, potentially with a merging galaxy or star formation present, which suggests this object has an irregular shape.
