The galaxy appears to be a relatively smooth, elliptical system. It exhibits a bright, concentrated central bulge with a distinct yellow hue, suggesting an older stellar population. The galaxy lacks prominent spiral arm structures or significant dust lanes. The overall shape is somewhat elongated, being slightly more oblong rather than perfectly spherical. There is a faint, diffuse halo surrounding the central region, exhibiting a bluer color shift. The faint blue shift in the halo suggests younger star formations in this peripheral region. Faint disturbances exist, potentially indicating minor tidal interactions or a past merger event.
