The galaxy presents as a single, relatively smooth, centrally concentrated object with a generally elliptical morphology. There is a slight elongation but it is mostly round. The galaxy appears to consist of two somewhat overlapping components; a more yellow component and a bluer component. The yellow component is brighter and slightly larger, possibly indicating an older stellar population. The bluer component is fainter and more compact.

Based on the morphology and colors, a possible interpretation is that this is a merging system consisting of two galaxies. One larger older galaxy (the yellow component) and one small younger galaxy (the blue component). There may be some active star formation occurring in the blue component. The overall appearance suggests this is an ongoing process with evidence of potential disturbance.
