The observed galaxy presents a predominantly elliptical morphology, although some features suggestive of a disk-like structure are also apparent. The central region exhibits a smooth, concentrated bulge, indicating a higher density of older stars. The galaxy displays a blue hue emanating from the outer regions, suggesting some ongoing star formation within a star-forming disk or spiral arms. However, no defined spiral arms are definitively discernible within the image. Overall, the light is generally redder than expected for a actively star forming system, and the blue light doesn't have a clear source such as HII regions, implying that it has low star formation activity. The galaxy appears relatively undisturbed, with no evidence of recent major mergers or significant tidal interactions. There might be some hint of a weak tidal arm.
