The galaxy presents as a somewhat disrupted system, appearing to be undergoing some form of interaction or merger. The primary body of the galaxy is elliptical in shape, with a smooth appearance, and a yellowish hue that suggests an older stellar population. A distinct secondary component is visible to one side of the main galaxy, appearing as a redder concentration of light, possibly indicating a region of active star formation.

The overall structure hints at an ongoing merger event, with tidal features that are subtle. The galaxy is of intermediate size and appears relatively massive. Based on its color and morphology, the galaxy likely exhibits a relatively low star formation rate overall, with concentrated activity possibly triggered by the interaction.
