The galaxy presents as a single, resolved object with an elliptical morphology. The galaxy exhibits a centrally concentrated luminosity profile, with intensity decreasing gradually towards the outer edges, suggesting a substantial bulge component. The light distribution appears relatively smooth, with minimal evidence of spiral arms or prominent dust lanes. The color gradient suggests a redder, more evolved stellar population, particularly in the central regions. The object appears slightly elongated, with a measured ellipticity implying a deviation from a perfectly circular shape. There are no obvious signs of ongoing major mergers or tidal disturbances in this image.
