The galaxy appears to be undergoing a significant merger event. The primary structure is diffuse and relatively smooth, yet clearly disturbed. There are at least two distinct, bright, compact nuclei or core regions. The overall morphology is highly irregular, lacking a clear spiral or elliptical structure. The color profile is dominated by redder hues, suggesting an older stellar population and/or significant dust obscuration. A faint, extended halo or tidal tail-like structure is tentatively visible, further indicative of gravitational interaction and disruption. There is minimal evidence of recent or ongoing star formation visible in the image. The galaxy has a relatively compact size.
