The galaxy presents as a moderately luminous object with a somewhat elongated, cigar-shaped morphology. Its light profile appears smooth with a slight hint of a disk structure. The color is consistent with a population of older stars, and it is likely undergoing a relatively low rate of star formation. There are hints of some disturbance or interaction, with minor asymmetry noticeable in the galactic structure, which suggest that it may be undergoing a merging event with another galaxy. 
