The galaxy presents a generally smooth morphology, exhibiting minimal signs of strong spiral arms or a distinct disk structure. The overall light distribution appears relatively uniform, with a slight elongation suggesting it is somewhere between a round and cigar shape. The color profile indicates a concentration of older stellar populations, evident in the reddish-yellow hue dominant throughout the galaxy's body, particularly within the central region. There is some evidence of minor disturbances in the surrounding area. The object seems to have intermediate brightness. It could be an elliptical galaxy in relative isolation.
