The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light profile. The morphology is generally smooth, with no obvious spiral arms or strong disk-like features. The main body of the galaxy has a slightly elongated shape, and a hint of tidal disturbance suggesting a possible ongoing or recent interaction, indicated by the faint plume like feature extending away from the main body of the galaxy. There also appears to be a secondary, smaller, but still noticeable concentration of light, potentially another galaxy, located near the primary object. The colors of the galaxy suggest a dominant population of older stars, as evidenced by its reddish-yellow hue. This indicates a relatively low star formation rate.
