The galaxy presents as a bright, elliptical structure, with a noticeable central bulge exhibiting a high surface brightness. The light distribution appears relatively smooth, suggesting an older stellar population dominates the galaxy. There is a slight elongation in the overall shape, deviating from a perfectly circular form. No distinct spiral arms or prominent dust lanes are visible within the image. The halo appears diffuse and extends some distance from the core. The colors suggest the presence of a mix of stellar populations, dominated by older, redder stars. There are no signs of any major mergers or significant tidal disturbances in the galaxy's morphology, suggesting it is a relatively undisturbed system. It is likely a relatively massive galaxy. The galaxy displays a moderate level of star formation.
