The galaxy presents as a centrally concentrated object with a smooth, diffuse light profile. The primary body exhibits a yellowish hue, indicative of an older stellar population. There is no apparent spiral structure or prominent dust lanes visible at this resolution, suggesting a lack of significant ongoing star formation. The galaxy appears to be largely spheroidal in shape, though not perfectly circular, showing a slight elongation. There are no visible signs of any major disturbances or mergers affecting the morphology. Faint extensions are present, but difficult to resolve. 
