The galaxy presents as a centrally concentrated object with a fairly smooth morphology. It appears somewhat elliptical in shape, exhibiting a high degree of symmetry. There is little evidence of spiral arm structure or significant dust lanes within the visible light. The color is subtly yellowish-white, suggesting an older stellar population with moderate star formation activity. There appears to be no major merger events or significant tidal disturbances. The estimated size is a few kiloparsecs, which indicates a dwarf galaxy that is slightly on the smaller side. The object is relatively isolated, without any obvious companion galaxies in close proximity.
