The galaxy appears as a diffuse, luminous object with a generally rounded morphology. It exhibits a smooth overall structure, suggesting a lack of prominent spiral arms or a well-defined disk component. The color profile indicates a significant population of older stars, with a reddish-yellow hue dominating the galactic light. There is a hint of a possible ongoing or recent merger event, suggested by some irregularities in the shape and light distribution. There is a somewhat clumpy appearance in the main body. There also seems to be an indication of some minor interaction or tidal disturbance in the upper left quadrant, which possibly represents a separate smaller galaxy. Based on the general appearance, it is likely a massive galaxy at a considerable distance.
