The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. The overall shape appears relatively round, lacking a distinct disk structure. There is a suggestion of a slightly disturbed structure, potentially indicating a past minor interaction or merger event. The galaxy exhibits a range of colors, with a yellow-white core and greenish hue in the outer regions. This could be a result of differing stellar populations, with older, redder stars dominating the core and younger, bluer stars in the surrounding areas. There is no spiral arm structure visible.
