The galaxy presents as a smooth, elliptical structure with a noticeable central bulge. The luminosity appears to be concentrated in the core region, gradually decreasing towards the outer edges. There is a subtle disk like appearance to the galaxy that does not appear highly disturbed. The overall color profile suggests a population of older stars, potentially with minimal ongoing star formation. No clear spiral arms or significant dust lanes are discernible within the resolution of the image. The galaxy does not seem to be undergoing a major merger, showing no dramatic tidal features or distortions. There is a minor irregularity on one side of the disk which could be evidence of a minor merger or tidal effects. The galaxy is elongated, appearing roughly twice as long as it is wide.
