This galaxy presents as a relatively compact, elliptical-like object, exhibiting a smooth and concentrated light distribution. The galaxy displays a dominant yellowish-orange hue centrally, suggesting an older stellar population. There is evidence of a redder region within the core of the galaxy, potentially indicative of dust obscuration or regions of more intense star formation. A faint, blueish halo is visible surrounding the galaxy, suggesting the presence of some younger stars. The overall morphology appears largely undisturbed, showing no signs of significant tidal interactions or ongoing mergers, although the galaxy appears to be interacting with another galaxy. The object displays a high degree of central concentration.
