This galaxy presents as a relatively smooth, rounded structure. The light distribution is centrally concentrated with a noticeable radial falloff. It appears to have a mostly homogenous color, skewed towards the green/yellow end of the spectrum. The lack of prominent spiral arms or dust lanes indicates that this may be an elliptical galaxy, or perhaps a spiral with a very tightly wound structure and low dust content. The galaxy appears to have undergone a merger in the past. The red component suggests the presence of a population of older stars, potentially contributing to the overall mass, however there are hints of recent activity. Overall the galaxy exhibits characteristics consistent with a galaxy that may have undergone some sort of transformation.
