The galaxy exhibits a complex morphology, indicative of a possible ongoing or recent merger event. It displays both smooth and featured components, with a dominant central region that appears relatively smooth. This central area emits strongly in the bluer wavelengths, suggesting a population of younger, hotter stars or possibly an active galactic nucleus.

There are extended features, some showing hints of spiral arm structures. A notable, elongated feature extends from the central region, exhibiting a redder color. This may be indicative of dust lanes or a population of older stars. The overall shape is somewhat cigar-shaped or elongated, not perfectly circular.

The visual characteristics suggest a galaxy with a relatively high stellar mass and ongoing star formation, but also significant contributions from an older stellar population. There is evidence that it may be interacting with another galaxy or undergoing internal disturbances that are influencing its shape and stellar populations.
