The galaxy presents as a centrally concentrated object with a smooth, largely featureless morphology. Its shape is generally elliptical, with a slight elongation apparent along one axis. The core exhibits a bright, concentrated luminosity, suggesting a high density of stars or potentially an active galactic nucleus. Moving outward from the core, the galaxy exhibits a diffuse halo, gradually fading into the background sky. The color profile indicates a dominant yellowish-red hue in the central region, possibly indicative of an older stellar population, while the outer regions show a slight blue tint, perhaps from the presence of younger stars or a small amount of ongoing star formation. No significant tidal features, dust lanes, or spiral arm structures are discernible, implying a relatively undisturbed evolutionary history. The absence of obvious morphological disturbances suggests a lack of recent major merger events. Overall, the galaxy appears to be a relatively massive, evolved system with a smooth light distribution.
