The galaxy presents as a somewhat elliptical-shaped object with a relatively smooth morphology. The central region exhibits a notable concentration of light. There is a slight indication of a possible disturbance or feature in the disk, and the slight color variation and possible clumping suggest some degree of ongoing star formation within the galaxy, which could contribute to the overall luminosity. The galaxy's color indices indicate it is a mid-luminosity object with a moderate mass. The observed light distribution is primarily uniform across the galaxy.
