The galaxy presents as a centrally concentrated, elliptical-like system. The light is dominated by a yellowish hue in the central region, suggesting an older stellar population. The galaxy appears relatively smooth with no distinct spiral arm structures or prominent dust lanes visible in this image. The outer regions of the galaxy exhibit a gradual fading of light, transitioning into the background sky, showing a high Sersic Index. There is a subtle blue tinge in some areas of the outer edges of the galaxy which could represent some star formation, although overall the galaxy is likely relatively passive. The shape is almost perfectly round with a very slight flattening. There is no evidence of any major ongoing merging activity.
