The galaxy presents as a moderately luminous object, exhibiting a generally smooth morphology. The overall shape is elongated, with a high degree of ellipticity, appearing cigar-shaped. There is some indication of a disk structure, though it is not sharply defined. The light distribution suggests a fairly homogenous stellar population throughout the galaxy, with perhaps a slight concentration of older stars toward the central region and a hint of bluer, younger stars distributed in a larger area. There may be a slight amount of tidal disturbance or interaction occurring, though this is not definitive.
