The galaxy appears as a centrally concentrated, ellipsoidal object. Its core exhibits a bright, yellowish-white luminosity, suggesting a population of older stars. This central region transitions smoothly outwards to a less intense halo of a somewhat bluer hue. No distinct spiral arms or bar structures are discernible in the image, suggesting that it may be classified as an elliptical galaxy. The overall smooth appearance, absence of significant dust lanes, and subtle color gradients further support this classification. There appears to be a slight distortion of the otherwise nearly circular shape, perhaps indicating a minor gravitational interaction.
