The galaxy presents a generally smooth morphology, with a high degree of central concentration. Its overall shape appears round. The central region exhibits a yellow-orange hue, suggesting an older stellar population. A faint blue-green halo surrounds the central region, possibly indicating a low level of on-going star formation. There is no discernable disk structure, spiral arms, or significant dust lanes are visible in this image. There appears to be no evidence of a major merger or tidal disturbances.
