The galaxy presents as a luminous, elliptical structure. Its central region exhibits a high degree of concentration, appearing smooth and largely featureless. The light intensity gradually diminishes from the core outwards, with the outer regions fading into the background sky. The galaxy's overall shape suggests a spheroidal morphology, with a slight elongation along one axis, although the degree of ellipticity is moderate. There are no readily discernible spiral arms or significant dust lanes apparent in this image. The galaxy's color appears relatively uniform across its surface, with a subtle shift toward redder hues in the central bulge. The lack of prominent blue regions suggests a relatively low rate of ongoing star formation. Overall, the galaxy appears to be a mature system, likely dominated by an older stellar population.
