This galaxy presents as a generally smooth, elliptical object with a concentrated central region. It exhibits a relatively high degree of symmetry and roundness. There is some evidence of a slight elongation. There appears to be a fairly even distribution of light throughout the galaxy, with a somewhat brighter core and a gradual fading towards the outer edges. The color profile suggests a population of older stars, given the lack of strong blue light indicative of active star formation. No prominent spiral arms, dust lanes, or other distinct features are discernible.
