The galaxy presents a generally smooth, elliptical morphology, showing little evidence of a spiral structure or prominent disk. The light distribution is highly centrally concentrated with a relatively steep decline in surface brightness away from the core. The central region exhibits a yellowish-white hue, suggesting an older stellar population dominating the core. There is a subtle color gradient transitioning to a slightly redder shade in the outer regions, which may indicate a difference in the age or metallicity of the stellar populations, with the outer parts containing older, redder stars. There is a hint of a very minor disturbance in the galaxy's form, though this could be due to image artifacts. The overall appearance is indicative of a relatively quiescent system, likely undergoing minimal star formation. The galaxy has a generally round shape.