The galaxy presents a smooth, elliptical morphology. It appears nearly circular, showing minimal elongation. The central region exhibits a bright, concentrated luminosity that fades gradually towards the outer edges. The color profile suggests an older stellar population, with a yellowish hue dominating the overall appearance. There is no visible evidence of spiral arms, dust lanes, or ongoing star formation regions within the galaxy's observed structure. The galaxy appears relatively undisturbed, with no signs of recent mergers or tidal interactions.
