The galaxy presents as a generally smooth, elliptical structure with a slight elongation or cigar shape. There is an indication of a minor disturbance or possible interaction, manifested as a faint, diffuse bridge of light extending between two brighter, more compact regions within the overall galactic structure. The primary body exhibits a core region with a redder hue, suggesting an older stellar population. The extended regions show bluer tones, implying the presence of younger, hotter stars or ongoing star formation, though at a relatively low rate. Overall, the galaxy appears to be an evolved system, possibly undergoing a minor merger event.
