The galaxy presents as a somewhat elongated, elliptical morphology. The light distribution appears relatively smooth, concentrated towards the center, with a gradual decrease in intensity towards the outer regions. There is minimal evidence of significant disk features or spiral arms. The central region exhibits a bright core, likely indicative of a dense stellar population or an active galactic nucleus. The overall color profile suggests a lack of significant ongoing star formation, trending towards a redder, more evolved stellar population. There might be some minor disturbances or faint tidal features, however, they are not prominent and difficult to discern with clarity. No signs of major merger activity are immediately apparent.
