The galaxy presents an overall elliptical morphology, appearing relatively smooth and exhibiting a high degree of central concentration. The light distribution suggests a dominant spheroidal component. The core region exhibits a yellowish hue, potentially indicating an older stellar population. Moving outward from the core, the color shifts towards a redder tone, possibly from dust extinction or older stars. The overall structure appears relatively undisturbed with no clear signs of spiral arms or significant tidal features. There is a redder region on the top left of the galaxy which may be a smaller, irregular galaxy undergoing a minor merger with the main galaxy.
