The galaxy presents as a relatively smooth, elliptical structure. Its central region exhibits a high degree of concentration, appearing bright and nearly spheroidal. Progressing outwards, there appears to be a disk-like component. The galaxy appears cigar shaped in the image. There is no visible evidence of active merging or tidal disruptions, with the majority of classifications indicating no major disturbances. The galaxy appears to be isolated and undisturbed. A smooth appearance may also be due to the resolution.
