The observed galaxy presents as a single, relatively smooth, and centrally concentrated object. The morphology appears elliptical, with a high degree of circularity. There is no obvious disk structure, spiral arms, or bar features visible. The light distribution is centrally peaked with a smooth falloff in intensity towards the outer regions.

The galaxy exhibits a yellow-orange hue, suggesting a stellar population dominated by older, redder stars. This color profile is consistent with an early-type galaxy undergoing relatively little current star formation. There are no prominent signs of dust lanes or active star-forming regions within the galaxy. No significant tidal disturbances or interactions with companion galaxies are apparent in the image.
