The galaxy appears to be a relatively smooth, elliptical galaxy. The core exhibits a bright, concentrated luminosity, suggesting a high density of stars in the central region. There is a slight elongation, indicating a deviation from a perfectly circular shape. The color distribution is somewhat uniform, with a central yellowish hue grading into a blueish outer region. There may be some faint disk-like structure, or perhaps a lens or bar structure, but it is difficult to distinguish in the image. There are no obvious signs of spiral arms or significant dust lanes. There is no apparent ongoing major merger activity, although some minor disturbance or irregularity cannot be completely ruled out based solely on this image. The light emitted indicates a notable stellar mass, and some star formation activity, though the specific star formation rate is not evidently high given the overall smooth morphology.
