The galaxy presents as a relatively compact object, exhibiting a smooth, elliptical morphology. The light profile appears centrally concentrated, with a bright, unresolved core indicating a significant bulge component. There is a lack of discernible spiral arms or prominent dust lanes within the galaxy's structure. The overall color is subtly shifted towards the redder end of the spectrum, suggesting a stellar population that is dominated by older, redder stars. No strong evidence of recent or ongoing major merger events is apparent in the image, although subtle distortions cannot be ruled out.
