The galaxy appears to be an elliptical type, exhibiting a smooth, concentrated distribution of light. The light is more concentrated towards the center and dissipates further from the center of the galaxy. The overall shape appears more akin to an in-between shape and not quite round. There appears to be a lack of pronounced spiral arms or prominent dust lanes. The color gradient suggests the presence of an older stellar population, potentially with ongoing, but relatively low star formation activity. No obvious signs of interaction or merging are visible. The galaxy shows a slightly reddish hue.
