This galaxy appears to be a relatively smooth, centrally concentrated system. The morphology is generally elliptical, exhibiting a soft, diffuse glow with no readily apparent spiral arm structures or distinct features. The color profile suggests a population of older stars, primarily emitting in the redder portions of the spectrum, with some possible contribution from younger, bluer stars creating a less intense glow. This galaxy does not show signs of recent major merger events or significant tidal disturbances.
