The galaxy presents as a relatively faint and compact object. Its overall structure appears complex and disturbed, possibly indicative of ongoing or recent interaction with another galaxy. There is no obvious spiral arm structure or a clear, well-defined disk. A central, somewhat elongated, and moderately bright core is visible. Emanating from the core are faint, diffuse extensions or tidal tails that appear asymmetrical, suggesting gravitational disruption. The galaxy exhibits a range of colors, with the core displaying a bluer hue, while the outer regions and tidal features showing more reddish tints. This color variation could indicate differing stellar populations, with the core potentially hosting younger, hotter stars, and the outer regions being dominated by older, cooler stars, or dust reddening of background starlight. There is evidence of an active galactic nucleus.
