The galaxy presents a notable smoothness in its overall appearance. Its morphology appears largely elliptical, tending towards a more circular shape, though some deviation from perfect roundness is observable. There are no definitive signs of prominent spiral arms or a well-defined disk structure. The galaxy appears to be relatively undisturbed, showing minimal evidence of ongoing or recent major merger events. There are subtle irregularities or minor disturbances that could be indicative of past interactions or accretion events. The light distribution suggests a fairly well-mixed stellar population with the possibility of a slight color gradient toward the center. The overall color of the galaxy leans toward the redder end of the spectrum, consistent with an older stellar population, although some bluer regions suggest the presence of some younger, hotter stars. 
