The galaxy presents a somewhat irregular morphology. The light distribution is centrally concentrated but extends asymmetrically, suggesting ongoing or recent interactions. The color profile appears predominantly blue, indicating the presence of a relatively young stellar population and ongoing star formation, particularly in the less centrally condensed areas. The overall structure hints at a potentially disrupted or merging system, lacking a clear spiral or elliptical form. Faint tidal features may be present, but deeper observations would be needed to confirm these. The apparent size suggests a dwarf galaxy. 
