The galaxy appears to be an elliptical galaxy, exhibiting a smooth, featureless morphology with a high degree of roundness. The central region presents a bright, concentrated core, potentially indicative of an older stellar population. A slight extension or halo of fainter luminosity surrounds the core, gradually fading into the background sky. Some bluer colors present, suggestive of star formation, however the galaxy remains dominated by older stellar populations. No evidence of spiral arms, bar structures, or significant dust lanes is readily apparent in this image. There are no obvious signs of an ongoing major merger event. However, there may be a minor disturbance.
