The galaxy appears as a centrally concentrated, relatively smooth structure with a slightly elongated morphology. The light profile suggests a dominant spheroid component, exhibiting a diffuse, elliptical glow. There is little evidence of spiral arm structure or significant dust lanes. The color is generally bluish-white in the central region, potentially indicating a population of younger, hotter stars, although the overall faintness suggests that it's composed of an older stellar population. There are no signs of tidal tails or major disturbances in the image, indicating it is an isolated system that is undisturbed. This galaxy is undergoing only very little star formation.
