The galaxy presents as a somewhat amorphous, yellowish-orange structure with a relatively smooth appearance. Its overall shape is elongated, though not strongly cigar-shaped. There is evidence of a possible merger or interaction, as suggested by the apparent dual or disturbed core region, exhibiting two primary concentrations of luminosity. The light distribution is concentrated towards the center with a gradual decline towards the edges. There may be a very faint, diffuse tidal tail structure emanating from the main body. 
