The galaxy presents as a relatively smooth, elliptical-like structure. Its core region exhibits a concentrated luminosity gradient, appearing a yellow-gold hue. This suggests a population of older stars in this region, with possibly lower ongoing star formation. Moving outward from the core, the galaxy's luminosity gradually decreases, and the color shifts toward a bluer tint. This may indicate the presence of a younger stellar population at the edges. The general shape is more "in between" round and elongated, meaning it is not perfectly spherical. I do not see any clear evidence of ongoing major mergers or strong tidal disturbances. The galaxy does not appear to have prominent spiral arms or a well-defined disk structure.
