The galaxy presents as a centrally concentrated elliptical object, exhibiting a smooth, relatively featureless morphology. Its overall color index suggests an evolved stellar population, leaning towards redder hues. The core region appears bright, with the light intensity gradually diminishing towards the outer edges. There is no apparent spiral structure or significant dust lane obscuration visible in this image. The galaxy's shape approximates an oblate spheroid, deviating slightly from a perfectly circular profile. There is little evidence of ongoing major star formation activity. The morphology is consistent with a galaxy that has undergone significant dynamical relaxation. No obvious signs of tidal interactions or recent merger events are apparent.
