The galaxy presents as a single, concentrated object with a smooth and relatively featureless profile. Its overall shape appears to be elliptical or spheroidal, displaying a high degree of roundness. The central region exhibits a yellowish hue, possibly indicative of an older stellar population dominating the core. Fainter blue-ish regions surround the core. These may suggest ongoing, albeit relatively low levels of star formation activity at the outskirts. There is no obvious evidence of spiral arms or a well-defined disk structure. Similarly, there are no apparent tidal tails, bridges, or other signs of recent or ongoing major merger events. The galaxy appears largely isolated and undisturbed in this image.
