The galaxy presents a generally smooth morphology with a slight elongation, suggesting a possible transition between elliptical and lenticular types. Its color profile indicates a dominant population of older stars, particularly within the central bulge, exhibiting a yellowish hue. There is a hint of bluer light in the outer regions suggesting some ongoing, albeit low-level, star formation. No distinct spiral arms or bar structures are discernible. The overall structure appears relatively undisturbed, lacking any significant signs of tidal interactions or major mergers. The galaxy exhibits a moderate degree of central concentration, with the light intensity decreasing gradually from the core outwards.
