The galaxy presents as a centrally concentrated object with a generally smooth appearance. It is not perfectly spherical, displaying a slightly elongated, intermediate shape. There are some subtle hints of internal structure, but the overall impression is of a relatively homogenous light distribution. No distinct spiral arms or prominent features are visible. The galaxy exhibits a predominantly blue-ish hue at its center and slightly redder at its very distant edge indicating the possibility of ongoing, but relatively low-level star formation activity. There is no evidence of significant tidal disturbances or a major ongoing merger. The overall morphology suggests that this galaxy could be a spiral or irregular galaxy at a great distance. 
