The galaxy presents a morphology consistent with a merging system. Two distinct components are visible, each exhibiting a relatively smooth appearance. The larger component is elongated, presenting an elliptical shape with a dominant reddish hue toward its core, suggestive of an older stellar population. A fainter, extended halo surrounds this core. The secondary component is located in close proximity to the primary. It exhibits a more compact and somewhat irregular shape with a bluish tint, which indicates ongoing star formation or a younger stellar population. Both components appear to be interacting gravitationally, as evidenced by a faint tidal feature or bridge of material connecting the two, indicating a merger in progress. Overall, the system appears to be relatively massive, with each component contributing significantly to the overall luminosity.
