The galaxy presents as a relatively smooth, elliptical-like structure. A concentrated, bright, yellowish core is evident, suggesting a significant population of older stars. Moving outward from the core, the color transitions subtly to a redder hue, indicating a possible decrease in stellar age and/or an increase in dust content in the outer regions. No distinct spiral arms or bars are visible. There is a very slight asymmetry in the outer halo which could indicate a minor tidal disturbance, although it could also be due to image artifacts. The morphology suggests a system undergoing relatively low levels of star formation.
