The galaxy presents as a centrally concentrated elliptical type. Its overall morphology appears smooth, with a notable absence of spiral arm structures or distinct dust lanes. The core region displays a high surface brightness, appearing nearly spherical and exhibiting a yellowish hue, possibly indicating an older stellar population. Moving outwards from the core, the galaxy gradually fades into a less luminous halo with a more elongated shape. This outer region exhibits a subtle color gradient, transitioning towards slightly redder tones. The overall color profile suggests a system dominated by evolved stars, with limited ongoing star formation. No significant tidal features or signs of recent major mergers are immediately apparent, supporting the classification as a relaxed elliptical galaxy.
