The galaxy presents as a largely smooth, centrally concentrated object with a generally elliptical morphology. The galaxy exhibits a dominant yellowish hue, indicative of an older stellar population. There is a small amount of asymmetry and potential disturbance visible, but not enough to categorize this as an active merger. There is some evidence of residual star formation. The galaxy's light profile suggests the presence of an extended halo, which appears to have some minor disturbances within it.