The galaxy presents as a centrally concentrated, generally smooth object. The core exhibits a reddish hue, suggesting an older stellar population and/or significant dust obscuration. The light profile appears fairly symmetrical and elliptical, displaying a high degree of roundness. There is little evidence of spiral arm structure or significant star formation regions within the visible extent. The overall morphology indicates a relatively undisturbed system, and shows a minimal presence of tidal features or signs of a recent major merger. There appears to be a subtle color gradient, transitioning from a redder center to slightly bluer outskirts, which could indicate some ongoing, albeit low, level of star formation in the outer regions. The galaxy exhibits a moderately high mass and low specific star formation rate, further supporting the conclusion that it is a relatively evolved, passive system.
