The galaxy presents a largely smooth, elliptical morphology. It exhibits a centrally concentrated light profile, suggesting a high degree of sphericity and a possible lack of significant disk-like structure. The dominant color is a reddish hue, suggestive of an older stellar population and a relatively low ongoing star formation rate. There appears to be evidence of a possible merger or tidal interaction as the edges of the galaxy appear diffuse and there are two distinct light sources with a slight bridge of material. These signs of galactic interaction could be indicative of morphological disturbance. 
