The galaxy appears to be undergoing a significant interaction, possibly a merger. There are two distinct luminous components, with the larger, more diffuse component showing a generally smooth appearance. This primary component exhibits a somewhat irregular shape, deviating significantly from a perfect ellipse or disk. The overall structure is rather amorphous with no clear spiral arms or bar structure.

The smaller, secondary component is more compact and exhibits a bluer color indicative of younger stellar populations. There may be a tidal feature connecting the two components, suggested by a faint extension between the two, but the feature itself is not clearly resolved in this image. This could be the result of a disruptive event such as a collision with another galaxy. A slight asymmetry in the larger component could also indicate past or ongoing interactions.
