The galaxy presents as a system exhibiting a combination of features, suggestive of an ongoing interaction or merger. It appears as a somewhat elongated object, with a brighter, more condensed central region displaying a yellowish hue. This central area likely represents the galaxy's core, potentially dominated by an older stellar population.

Extending away from the primary body is a fainter, more diffuse component, potentially indicative of tidal debris or disrupted spiral arms. This component exhibits a slightly bluer coloration compared to the core, possibly hinting at more recent star formation within these disturbed regions.

There is evidence of a secondary nucleus or a concentration of stars separate from the main bulge, suggesting an interaction with another galaxy. The overall morphology deviates significantly from a classical elliptical or spiral, indicating a dynamically active system.
