This galaxy appears to be elliptical in nature, exhibiting a generally smooth and concentrated light distribution. The morphology leans towards a rounded shape, but with a slight elongation visible. There is no obvious presence of spiral arms or significant disk structure. The central region is noticeably brighter, suggesting a prominent nucleus or bulge. There may be minor disturbances within the galactic structure, but no major merging activity or strong tidal features are immediately apparent. The overall color profile displays a redder hue in the central regions, transitioning to bluer colors in the outer areas. This could indicate a population of older stars in the center and younger stars in the periphery.
