The galaxy presents as a centrally concentrated object, exhibiting a generally smooth morphology. The light distribution appears relatively even across its body, with a noticeable increase in intensity toward the core. There is a subtle elongation observed, suggesting a possible elliptical shape or a disk galaxy viewed at an angle. The central region shows a yellowish hue, potentially indicating an older stellar population, while the outer regions exhibit a bluer tint, hinting at the presence of younger stars and possibly some ongoing star formation. There may be some minor disturbances within the galaxy's structure or perhaps some features indicative of past interactions. No pronounced spiral arms or distinct dust lanes are discernible in this image. The overall impression is that of a mature galaxy.
