The galaxy appears as a centrally concentrated object with a relatively smooth, rounded morphology. Its core exhibits a bright, yellowish-orange hue, suggesting a population of older stars. There is little evidence of defined spiral arms or significant substructure. The overall color profile indicates a red sequence galaxy, potentially an elliptical or lenticular type. The light distribution appears fairly uniform, diminishing gradually from the core outward, with no sharp edges or distinct features disrupting its smooth appearance. There does not appear to be any ongoing major merger events or significant tidal disturbances affecting the system's overall structure.
