The galaxy presents as a dual system, likely in interaction or close proximity. The first galaxy exhibits a relatively smooth, elliptical morphology, appearing largely featureless. Its color profile skews towards redder wavelengths, suggestive of an older stellar population and potentially a lower rate of ongoing star formation.

The second galaxy displays a bluer color profile, indicating the presence of younger, hotter stars and active star formation regions. Its shape is less defined, possibly due to tidal distortion from gravitational interactions. It appears slightly more extended than the redder galaxy.

Given the projected proximity and signs of possible disturbance, this system could be a pre-merger.
