The galaxy presents as a relatively smooth, concentrated object with a dominant central bulge. The overall morphology appears elliptical or lenticular, exhibiting a high degree of circularity. There is little evidence of spiral arms or significant disk features. The color gradient is subtle, with the core appearing slightly more yellow or red than the outer regions. The light is concentrated and gradually fades from the core out, without large changes in magnitude. The overall structure suggests a galaxy that has undergone significant evolutionary processes, potentially resulting in a well-mixed stellar population and depletion of gas reservoirs for ongoing star formation. There is no clear evidence of ongoing major mergers or tidal disturbances, although some minor irregularities in the outer halo cannot be entirely ruled out at this resolution. The galaxy's structural properties and color are broadly consistent with a system that has undergone substantial quenching of star formation activity.
