The galaxy exhibits an elliptical morphology. The light profile appears smooth and centrally concentrated, with a noticeable color gradient. The core region displays a yellowish hue, potentially indicating a population of older stars. Moving outward, the color shifts towards a slightly bluer tone, suggesting the presence of a younger stellar population in the outer regions. The galaxy appears elongated, indicating a non-spherical shape, with a cigar like appearance. There is no evidence of prominent spiral arms or a distinct disk structure. There are no noticeable tidal tails or signs of major mergers in this image, but there could be a minor disturbance occuring.
