The galaxy presents a primarily smooth morphology, appearing somewhat elliptical in shape, though exhibiting some degree of irregularity. There is a notable concentration of light in the central region, indicating a bulge-dominated system. The color gradient suggests a significant population of older stars, resulting in a redder appearance, particularly within the core. Evidence of some bluer regions indicates a potential, albeit limited, presence of younger stellar populations and ongoing star formation. The overall structure appears relatively undisturbed, with no obvious signs of a major recent merger event. The galaxy's faint, extended halo could possibly be the result of previous accretion events or interactions.
