The galaxy presents as a relatively smooth, centrally concentrated object. Its overall form is elliptical, appearing only slightly elongated. The core exhibits a bright, diffuse glow, suggesting a dense stellar population. The galaxy shows some evidence of interaction with a secondary body, which is smaller in size and of a redder hue. It is unclear if the redder object is a companion galaxy undergoing a tidal interaction with the primary galaxy, or a background object gravitationally lensed by the foreground mass of the larger galaxy. The main galaxy exhibits a color gradient, transitioning from a yellow-orange core to a slightly bluer outer halo, implying varying stellar populations and/or dust content. The presence of merger or tidal features further suggests a dynamic environment, which could be stimulating star formation in the object.
