The galaxy appears to be a luminous elliptical. Its morphology is smooth and largely featureless, with a concentrated central bulge. The light profile indicates a high degree of radial symmetry. The galaxy exhibits a warm color profile, likely representing an older stellar population. It is more luminous in redder wavelengths, with fainter emission in bluer wavelengths. There is no evidence of spiral arms, dust lanes, or ongoing major mergers. A faint blue halo surrounds the central region. There are no signs of tidal tails or strong gravitational disturbances.
