The galaxy presents as a diffuse, moderately luminous object. Its overall morphology appears somewhat irregular and extended, not exhibiting a clear spiral or elliptical structure. The light distribution within the galaxy is uneven, with a central, brighter region. A faint arm-like extension is observable, possibly indicating ongoing gravitational interactions or tidal disruption. Color gradients suggest the presence of varying stellar populations and dust content within the galaxy. The bluer hues on the edges indicate areas of potential star formation. The overall appearance suggests a galaxy undergoing interaction or recent merger.
