The galaxy appears as a centrally concentrated, luminous object with a roughly elliptical morphology. The core region exhibits a bright, concentrated glow, indicative of a dense stellar population or potentially an active galactic nucleus. The outer regions of the galaxy fade gradually, forming a relatively smooth halo without prominent spiral arm structures. There may be slight disturbances or irregularities in the outer halo. The overall color profile suggests a population of older stars, potentially indicating a galaxy that has largely ceased active star formation. The galaxy is generally round in shape, without major asymmetry. The structure does not show signs of a major merger event.
