The galaxy presents as a single, centrally concentrated light source. It exhibits a smooth, largely featureless morphology, with a generally elliptical shape. The core region appears as a bright, slightly diffuse glow, suggesting a concentration of older stellar populations. There are no visible spiral arms or distinct disk-like structures. A very slight color gradient exists, trending towards slightly redder hues in the core, transitioning to slightly bluer color towards the outer regions. This could indicate some recent or ongoing star formation, but at a low rate. There is no evidence of significant mergers or tidal disturbances. The overall appearance is consistent with an elliptical galaxy with a relatively large mass and low star formation activity.
