The galaxy appears as a centrally concentrated elliptical-like object. It exhibits a generally smooth morphology with a high degree of roundness. The light distribution is dominated by a yellowish core, indicating a population of older stars. Fainter, slightly bluer light extends outwards from the core suggesting the presence of younger star formation regions. There is no apparent spiral arm structure or significant dust lane obscuration visible in this image, nor any strong indication of an ongoing major merger event or strong tidal disturbances. The observed color and morphology suggest a relatively evolved system, plausibly a high-mass elliptical galaxy with a modest level of ongoing star formation.
