The galaxy appears as a moderately bright, elliptical-shaped object. It exhibits a relatively smooth, featureless morphology with no discernible spiral arms or bar structure. A slight elongation is visible, suggesting it is not perfectly spherical, appearing to be in between round and cigar-shaped. The color profile indicates a dominant population of older stars, shifting to a more white/yellow hue in the core of the galaxy. There is little evidence of significant dust lanes or recent star formation activity. Based on the shape, lack of spiral arms, and color, this appears to be an elliptical galaxy at redshift z ≈ 0.15. There are no obvious signs of an ongoing major merger, though minor disturbances cannot be ruled out.
