The galaxy presents as a relatively smooth, elliptical form. The light distribution suggests a central concentration, with a gradual decrease in surface brightness toward the outer regions. Color gradients are subtle, with a slightly redder hue concentrated in the core, potentially indicative of an older stellar population or dust obscuration. There is no apparent spiral structure or distinct features such as star-forming regions. The overall appearance implies a mature galaxy, likely with a reduced rate of ongoing star formation. There is very slight visual evidence of a minor disturbance.
