The galaxy presents as a centrally concentrated, elliptical morphology. Its overall form appears relatively smooth, with no immediately discernible spiral arm structures or prominent dust lanes. The core region is significantly brighter and exhibits a yellow-orange hue, suggesting an older stellar population dominating the central mass. Moving outwards from the core, the light intensity decreases gradually. There's a slight elongation to the galaxy's shape, departing from a perfectly circular profile. The outer edges of the galaxy fade smoothly into the background sky, with no sharp truncations or abrupt changes in luminosity. Based on these features, it's likely a relatively massive galaxy with a moderate amount of ongoing star formation.
