The galaxy presents a largely smooth morphology, with a significant fraction of its light concentrated in a central bulge. While there is some evidence of a surrounding disk, it is not sharply defined, appearing somewhat diffuse. The galaxy exhibits a slightly elliptical shape, closer to round than cigar shaped. The color distribution suggests a relatively older stellar population, particularly within the bulge, which displays a yellowish hue. There is faint blue light also apparent within the galaxy, suggesting an observable low level of current star formation. No major distortions or tidal features are apparent, and it is likely this galaxy is not currently undergoing a major merger, although there may be some indications of possible minor gravitational interactions from nearby systems. 
