The galaxy appears to be an elliptical galaxy, exhibiting a smooth, featureless morphology. The overall shape is elongated, but not highly so. The galaxy appears to be a relatively homogenous distribution of light, with a bright central region. There is no discernible spiral structure or prominent dust lanes. Color gradients across the galaxy are subtle, with a slightly yellower hue in the central region and a bluer hue in the outer regions. Based on these characteristics, the galaxy is likely composed predominantly of older stellar populations. There are no significant tidal features or other signs of recent major merger activity observed in the galaxy’s morphology, although there may be minor disturbance given the slightly off centered core.
