The galaxy exhibits a complex morphology suggesting a possible interaction or recent merger event. One section presents a relatively smooth, concentrated structure with a yellowish hue, possibly indicative of an older stellar population. A redder area is visible that may be indicative of the presence of dust. Connected to this, a more diffuse region extends outwards, displaying a bluer color. This region appears less structured, possibly a tidal tail resulting from gravitational interaction with another galaxy or remnant of a smaller galaxy that merged with the primary body. The overall shape appears somewhat elongated, although not strongly defined as a pure elliptical or spiral form.
