The galaxy presents as a generally smooth, elliptical morphology. It exhibits a relatively high degree of central concentration with a smooth decline in surface brightness moving outwards. The primary body of the galaxy is largely featureless, suggesting an older stellar population. The galaxy's color is largely homogenous, skewed toward the red end of the spectrum, indicative of a population of older, redder stars with minimal ongoing star formation. There appears to be a very slight elongation or asymmetry, possibly indicating a prior minor merger event, though it does not show distinct tidal features.
