The galaxy presents a relatively smooth morphology, with a slight central bulge that graduates into a disk component. The disk displays a bluish tint. There are no prominent spiral arms visible in this image, nor are there any obvious signs of ongoing major merger activity. The colors suggest that some star formation is occurring, but the galaxy may also contain a significant population of older stars, particularly within the central bulge. The overall impression is of a galaxy evolving in relative isolation. The light distribution appears relatively symmetrical.
