The galaxy presents as a primarily smooth and elliptical-like structure, exhibiting a concentrated central bulge and a gradual decrease in luminosity outwards. The galaxy appears to have an intermediate ellipticity, not perfectly spherical but not highly elongated either. It exhibits a dominant yellowish-orange hue, indicative of an older stellar population with minimal ongoing star formation. There is a hint of asymmetry, potentially suggesting a minor gravitational interaction or disturbance; this is subtle, not indicative of a major merger event. Overall, the galaxy's morphology suggests it is a relatively evolved system likely composed of older stars.
