The galaxy appears as a moderately bright, elliptical or lenticular system. It exhibits a generally smooth morphology, with no prominent spiral arms or distinct dust lanes visible in this image. The color profile suggests a population of older stars, as indicated by its relatively red hue. The galaxy's shape is somewhat elongated, showing a slight cigar-like form. There are no signs of active merging or major tidal disturbances apparent in the surrounding vicinity. This object is a considerable distance away, with a measured redshift suggesting substantial recessional velocity. The overall light distribution indicates a centrally concentrated structure, typical of early-type galaxies.
