The galaxy appears as a relatively bright, rounded structure, exhibiting a smooth light profile with no discernible spiral arms or bar. Its core region shows a gradual increase in luminosity towards the center. The color appears to be a yellowish-white hue, suggesting an older stellar population. There is no evidence of significant dust lanes or recent star formation activity. Its morphology is indicative of an elliptical galaxy. No signs of major mergers or tidal disturbances are visible, although there may be a slight asymmetry or minor disturbance in the outer regions. The galaxy appears to be relatively isolated within its immediate surroundings.
