The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. Color gradients suggest a slightly bluer core transitioning to redder outer regions. There is a lack of distinct spiral arms or prominent dust lanes, indicating an older stellar population. The galaxy's shape is generally rounded, with only minor deviations from a perfect circle. There is no visible evidence of ongoing merger activity or significant tidal disturbances. The overall morphology suggests a quiescent galaxy dominated by evolved stars, with a low star formation rate.
