The galaxy presents a complex morphology, exhibiting characteristics of both smooth and disk-like structures. A dominant spheroidal component is observed, displaying a relatively smooth and concentrated light distribution with a yellowish hue. This central region suggests an older stellar population, with diminished recent star formation.

Interacting with this primary structure is a less defined, bluer component appearing somewhat amorphous. This region displays less concentration, and its color indicates the presence of younger, hotter stars and ongoing star formation. There is a faint tidal feature or arm extending from the amorphous region, suggesting gravitational interaction.

Overall, the galaxy appears to be in a state of merger or strong interaction, with the differing morphologies and stellar populations indicating a complex formation history. Evidence of tidal disturbances further supports this hypothesis. The galaxy's apparent color suggests that the spheroidal component is more massive and dominant than the disk-like or irregular regions.
