The galaxy exhibits a relatively smooth morphology, with a dominant elliptical shape. The light distribution appears concentrated toward the center, and there seems to be an absence of distinct spiral arm structures. The color is primarily consistent with older stellar populations, revealing a yellow/red hue. There is a slight elongation to the galaxy's shape, though it could be classified as tending to be in between round and elongated. There is little evidence of active star formation and it is likely not undergoing a major merger. There may be a minor disturbance present.
