The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, with a high degree of roundness. The color profile suggests a dominant population of older stars, evident from the reddish-yellow hue, but with some younger bluer populations closer to the core.  There is no obvious evidence of spiral arms or a well-defined disk structure, but instead a homogenous body, potentially with some minor disturbances from the past. A bright core is visible, but the details are unresolvable in this image. The stellar mass is relatively high and star formation is happening, but at a relatively slow rate. The galaxy does not appear to be undergoing any major merging events or significant tidal distortions.
