The galaxy presents as a moderately inclined disk system. It appears to be undergoing significant interaction, potentially a major merger event, given the disturbed morphology. The central region exhibits a diffuse, elongated structure, possibly a tidal tail or bridge resulting from the interaction. The overall color profile suggests a mix of stellar populations, with some regions displaying redder hues indicative of older stars and dust, while other regions are more bluish, suggestive of younger, hotter stars. The overall appearance is not of a classical spiral or elliptical galaxy, but rather a system in transition due to the ongoing merger. There are signs of active star formation likely occurring as a consequence of tidal forces. It appears somewhat patchy across its length.
