This galaxy presents as a relatively smooth, elliptical-like structure, appearing mostly featureless. The galaxy's central region exhibits a bright, concentrated light, likely indicating a dense stellar population. The light distribution suggests that the galaxy is elongated, with a ratio of approximately 2:1 along its major and minor axes. The color gradient progresses from a yellowish-white core to a slightly bluer outer region. No pronounced spiral arms or distinct dust lanes are readily apparent in this image. There are some vague features and a very slight hint of a disk, but overall the galaxy is dominated by a smooth and centrally concentrated morphology. There is no evidence of a major ongoing merger. The presence of a yellowish core hints to the likely presence of older stellar populations, while the outer, somewhat bluer region possibly implies the presence of younger star formation regions.
