The galaxy appears to be a merging system, exhibiting a significant tidal interaction between two distinct components. The primary galaxy displays a smooth, elliptical morphology and is characterized by a bright, concentrated core and a diffuse, yellowish halo. There is some indication of a slightly irregular shape or extension within the central region. A secondary component, located in close proximity to the primary, appears smaller and more amorphous, possibly exhibiting tidal features or ongoing star formation. There is evidence of a possible tidal tail extending away from the interacting pair. The color profile indicates that the galaxy has a somewhat older stellar population with a lower abundance of recent star formation, primarily composed of redder colors, although there are some indications of bluer regions indicative of active star formation in the merging regions. The merger shows a notable feature possibly indicative of a significant merger in progress or a close interaction with tidal effects.
