The galaxy presents as a moderately luminous object with an apparent spheroid morphology. It appears largely featureless, lacking discernible spiral arms or a prominent central bar. The galaxy exhibits a concentrated central bulge that fades smoothly towards its outer regions. The color profile suggests a population of older stars, with a bias towards redder wavelengths. There is no indication of ongoing major star formation, and it does not show signs of significant tidal disturbances or interactions with other galaxies. It is relatively round in shape, but not perfectly so. There may be evidence of a small, very dim disk.
