The galaxy presents as a diffuse object with an apparent angular size of approximately 6.7 arcseconds. Morphologically, it is irregular, displaying disrupted features suggesting gravitational interactions. The galaxy's light profile is not smooth; it has clumps and extended structures indicating recent or ongoing star formation. Color gradients within the galaxy reveal a mixed stellar population, with bluer regions possibly representing younger stars and redder regions potentially indicating older stellar populations or dust extinction. There appears to be a slight tidal tail or stream extending from the main body of the galaxy, hinting at a possible merger event or close encounter with another galaxy. The core is not well-defined. Overall, this galaxy appears to be in a state of dynamic evolution.
