The galaxy presents as an elongated, elliptical structure. The central region exhibits a high concentration of luminosity, appearing smooth and featureless. The core color is predominantly yellow, indicative of an older stellar population likely dominated by evolved red giant stars. Moving outward from the core, the color profile shifts towards a blue hue. The edges of the disk structure are fading into the dark background, suggesting the galaxy has low levels of ongoing star formation, and exhibits a spiral disk. The lack of clearly defined spiral arms supports the inference of a relatively low star formation rate. There is no apparent dust lane obscuring the galaxy's nucleus, and no obvious signs of a major ongoing merger event. Overall, the galaxy appears to be a relatively quiescent, red-sequence galaxy with the presence of a spiral structure.
