The galaxy presents a complex morphology. It appears to be undergoing a significant interaction, possibly a merger. The main body of the galaxy exhibits a relatively smooth, elliptical profile, suggesting an older stellar population. However, there are noticeable disturbances in its structure, particularly in the form of extended tidal features or tails. These features exhibit a lower surface brightness and a bluer color, hinting at ongoing star formation. 

The central region is very bright, possibly indicative of an active galactic nucleus or a dense concentration of stars. The overall color of the galaxy is yellowish, which is typical for galaxies with an older stellar population, with some bluer patches around the outer edges, which is typical of younger stars.

The morphological classification would place this galaxy within the realm of interacting or merging systems, with evidence of both smooth components and disturbed features.
