This galaxy appears to be a relatively smooth, elliptical galaxy. It is characterized by a concentrated central bulge, emitting primarily in the yellow-red part of the spectrum. There is little evidence of spiral arms or significant dust lanes. The object exhibits a high degree of central concentration, with the light intensity decreasing gradually outward from the core. No distinct star-forming regions are visible, suggesting a low star formation rate. There's a slight ellipticity to the galaxy, as it appears somewhat elongated rather than perfectly circular, but it is primarily spheroid in shape. The outer edges are diffuse and lack clearly defined boundaries. There is some evidence of a slight asymmetry in the outer isophotes, though this could potentially be due to lower signal-to-noise in the image or a past minor interaction.
