The galaxy appears to be in a late-stage merger, displaying a disturbed morphology. Two distinct nuclei are visible, one appearing more diffuse and elongated than the other. The larger, more central nucleus exhibits a yellowish-orange hue, indicating an older stellar population. Faint extensions are present, potentially tidal tails or remnants of disrupted spiral arms, suggesting ongoing gravitational interactions. The overall structure is irregular, lacking a clear spiral or elliptical shape. The color profile suggests a relatively low rate of ongoing star formation, although there may be localized pockets of more recent activity.
